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	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1476</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1476"/>
		<updated>2012-12-14T17:35:21Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Wavelength */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription for more details.&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range, the actually available monochromatic energy range is restricted to energies below 20 keV due to the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The remaining non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle (software).&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. The grid is also used to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
PBBA (para-brome benzoic acid) is used as scatterer at the sample position (e.g. in a capillary or as powder on a film). &lt;br /&gt;
Calibration of the beam center, distance and detector inclinations is done by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1475</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1475"/>
		<updated>2012-12-14T17:34:40Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription for more details.&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The remaining non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle (software).&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. The grid is also used to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
PBBA (para-brome benzoic acid) is used as scatterer at the sample position (e.g. in a capillary or as powder on a film). &lt;br /&gt;
Calibration of the beam center, distance and detector inclinations is done by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1474</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1474"/>
		<updated>2012-12-14T17:34:15Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* WAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The remaining non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle (software).&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. The grid is also used to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
PBBA (para-brome benzoic acid) is used as scatterer at the sample position (e.g. in a capillary or as powder on a film). &lt;br /&gt;
Calibration of the beam center, distance and detector inclinations is done by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1473</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1473"/>
		<updated>2012-12-14T17:32:19Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Pixel Size */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The remaining non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle (software).&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. The grid is also used to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1472</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1472"/>
		<updated>2012-12-14T17:31:34Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Detector Response/Flat Field */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The remaining non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle (software).&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1471</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1471"/>
		<updated>2012-12-14T17:31:00Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Detector Response/Flat Field */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The remaining non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1470</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1470"/>
		<updated>2012-12-14T17:30:23Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Absolute Intensity */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector efficiency.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1469</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1469"/>
		<updated>2012-12-14T17:29:46Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Absolute Intensity */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
any other calibration factor, e.g. the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1468</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1468"/>
		<updated>2012-12-14T17:29:06Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Wavelength */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is restricted to energies below 20 keV by the mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1467</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1467"/>
		<updated>2012-12-14T17:28:15Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
Setup optimized for 12.6 keV.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole energy range accessible by the monochromator, the actually available monochromatic energy range is reduced to Emax=20 keV by the reflecting mirror) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1466</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1466"/>
		<updated>2012-12-14T17:25:30Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube (distances 0.8 m to 10 m).&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole accessible energy range) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1465</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1465"/>
		<updated>2012-12-14T17:24:36Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* SAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole accessible energy range) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero diameter (accuracy &amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1464</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1464"/>
		<updated>2012-12-14T17:23:02Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
Monochromatic X-ray pinhole camera with 10 m vacuum flight tube.&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole accessible energy range) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero size (&amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1463</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1463"/>
		<updated>2012-12-14T17:22:03Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
10 m X-ray scattering tube&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole accessible energy range) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero size (&amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1462</id>
		<title>Calibration Procedures</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=Calibration_Procedures&amp;diff=1462"/>
		<updated>2012-12-14T17:21:32Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: /* Summary of Calibration Procedures */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;=Summary of Calibration Procedures=&lt;br /&gt;
In order to share good practice and information about different procedures the following page provides summaries as to how small-angle scattering instruments are calibrated as regards wavelength, intensity, momentum transfer and other quantities,  We encourage people to fill in details and make comments on this page.  In order to simplify finding information, we encourage everyone to use similiar sub-headings where appropriate.&lt;br /&gt;
&lt;br /&gt;
This project to gather information is new and we hope to have some information soon.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Quokka - Bragg Institute, ANSTO==&lt;br /&gt;
&lt;br /&gt;
40 m Small-angle neutron scattering instrument&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
&lt;br /&gt;
==ESRF ID02 Time-resolved SAXS/WAXS/USAXS/ASAXS==&lt;br /&gt;
&lt;br /&gt;
see also http://www.esrf.fr/UsersAndScience/Experiments/SoftMatter/ID02/BeamlineDescription&lt;br /&gt;
&lt;br /&gt;
(draft version)&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
Global calibration of the monochromator (over the whole accessible energy range) at different absorption edges and least square refinement of dBragg and thetaOffset over all scanned edges: Fe K-edge, Cu K-edge, Au LIII-edge, Zr K-edge, Mo K-edge, Rh K-edge (error DeltaE/E &amp;lt; 10^-4).&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity===&lt;br /&gt;
We are using the small angle scattering of water to determine a normalization factor that adjusts the online corrected intensity. This calibration factor supersedes&lt;br /&gt;
the intensity calibration of the beam intensity monitors and the detector sensitivity.&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
The detector uniformity is determined with fluorescence radiation. The detector is placed in 1 m - 2 m distance from the fluorescent sample. The non-uniformity of the field (&amp;lt;0.25% for a 10 cm x 10 cm active area) is corrected by normalizing the intensity pattern to the spherical angle.&lt;br /&gt;
For calibrations around 12 keV we use the K-alpha radiation of bromine at 11.9 keV (solution of HBr in water filled into a 3 mm thick glass capillary). The average value of the resulting flat-field pattern is normalized to unity (for convenience).&lt;br /&gt;
&lt;br /&gt;
===Pixel Size===&lt;br /&gt;
The pixel size is measured with a calibration grid in front of the detector. This is also to determine and to correct image distortions, e.g. when using fiber optically coupled CCD detectors.&lt;br /&gt;
&lt;br /&gt;
===Sample to Detector Distance===&lt;br /&gt;
====SAXS====&lt;br /&gt;
The movement of the detector is encoded. To calibrate the distance of a reference position from the detector a sample is placed there (e.g. silverbehenate or any other sample showing well defined rings, the d-spacing is not needed here). Then a series of scattering patterns is taken for different detector positions and the rings are extrapolated to zero size (&amp;lt;10^-3) which gives the position of the reference sample. The distance of any sample from the detector is measured relative to the reference position with a ruler (typically 1 mm accuracy). The center is determined with a scattering sample that is permanently present in the setup and that can be inserted into the beam path.&lt;br /&gt;
====WAXS====&lt;br /&gt;
Using PBBA (para-brome benzoic acid) as scatterer at the sample position (e.g. in a capillary or as powder on a film).&lt;br /&gt;
Calibration of beam center, distance and detector inclinations by a least square refinement. This refinement can also be used for SAXS.&lt;br /&gt;
&lt;br /&gt;
===Center===&lt;br /&gt;
The beam center and/or point of normal incidence is determined with a reference sample showing a circular scattering pattern (see above).&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;br /&gt;
Usually, the standard calibration is sufficient. If needed, additional fine adjustments can be done with reference samples.&lt;br /&gt;
&lt;br /&gt;
==Another Instrument==&lt;br /&gt;
&lt;br /&gt;
===Wavelength===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Absolute Intensity=== &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Detector Response/Flat Field===&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Comments about advantages/problems===&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=931</id>
		<title>2012 Data Discussion</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=931"/>
		<updated>2012-07-19T09:26:00Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;*The following is the agenda of work posted under business for [[canSAS-2012]].  Please add comments here:&lt;br /&gt;
** &#039;&#039;&#039;1D Format&#039;&#039;&#039;&lt;br /&gt;
** agree a proposed foreign namespace extension of the current 1D standard (required to enable, for example, t-o-f instruments to store auxillary wavelength-dependent non-I(Q) data in the same output files)&lt;br /&gt;
*** see Section 1.6.5 in [http://svn.smallangles.net/trac/canSAS/browser/1dwg/tags/v1.0/doc/cansas-1d-1_0-manual.pdf?format=raw here]&lt;br /&gt;
*** and look at this [http://svn.smallangles.net/trac/canSAS/browser/1dwg/data/Glassy%20Carbon/ISIS/GLASSYC_C4G8G9_withTL.xml example]&lt;br /&gt;
*** or [http://www.smallangles.net/wgwiki/images/f/f5/ISIS_SASXML_v1_1_Monitor_Spectrum_Example.XML this] one&lt;br /&gt;
** agree resultant changes to the schema/stylesheet&lt;br /&gt;
    SMK  - For clarity, this extension was proposed &#039;&#039;after&#039;&#039; adoption of the existing version of the standard. Ratification of&lt;br /&gt;
           this extension at CanSAS-2012 would give facilities/software developers the necessary confidence to implement it.&lt;br /&gt;
    SMK  - This proposed extension would allow more-or-less any non-I(Q) data to be included in a CanSAS-1D data file under a&lt;br /&gt;
           suitable foreign namespace. That is remarkable flexibility, and it does not require any significant revision&lt;br /&gt;
           of the existing standard. However, it could be argued that certain types of non-I(Q) data are so integral to a SAS&lt;br /&gt;
           experiment that they should instead be given explicit SASXML tags within the standard? Transmission data is a good&lt;br /&gt;
           example of this: the existing standard explicitly includes a tag for the transmission value from a &#039;&#039;monochromatic&#039;&#039;&lt;br /&gt;
           measurement (SASsample\transmission) but makes no provision for transmission values from &#039;&#039;white beam&#039;&#039;&lt;br /&gt;
           measurements. The proposed foreign namespace extension will make such provision possible &#039;&#039;but only&#039;&#039; as an&lt;br /&gt;
           extension, not as a formal part of the standard. Is that acceptable? The downside of explicitly adding new SASXML&lt;br /&gt;
           tags to the existing standard is that it would require issuing a new version of the standard. &lt;br /&gt;
    ARJN - I would recommend that during this meeting that the current format then be &#039;parked&#039;, the new 2D format&lt;br /&gt;
           should be flexible enough to handle 1D and 2D data.&lt;br /&gt;
    SMK  - Agreed.&lt;br /&gt;
    ARR  - Perhaps we should be cautious about suggesting no further development for the existing 1-D format. Unless&lt;br /&gt;
           there is scope for adapting to future needs, it will be seen as not suitable for new uses.  This, of course,&lt;br /&gt;
           does not imply that there have to be active plans for further changes at present. &lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
** &#039;&#039;&#039;2D Format&#039;&#039;&#039;&lt;br /&gt;
** define minimum necessary for reduced data&lt;br /&gt;
*** review previous discussions on 2D&lt;br /&gt;
*** considerations specific to 2D reduced data&lt;br /&gt;
*** consider forward looking issues such as &lt;br /&gt;
**** grazing incidence&lt;br /&gt;
**** event mode analysis&lt;br /&gt;
** suggest format framework (NeXus extension, canSAS 1D extension, other) with brief discussion of the reason for the choice (including options considered, pros and cons of each, and final weighing)&lt;br /&gt;
*** compare with NeXus definitions for:&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas &#039;&#039;&#039;NXsas&#039;&#039;&#039;]&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXiqproc &#039;&#039;&#039;NXiqproc&#039;&#039;&#039;]&lt;br /&gt;
** Guide to how to make implementation easy.&lt;br /&gt;
** Create straw format suitable for test/demonstration use and convert some test data for such a demonstration.&lt;br /&gt;
** Provide a plan for presentation at SAS 2012&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
* A proposal for a 2D version of the canSAS 1D data format has been posted for discussion: [[2D Data Format Proposal]]&lt;br /&gt;
* NeXus has a definition for multi-dimensional data:&lt;br /&gt;
** http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas&lt;br /&gt;
** http://svn.nexusformat.org/definitions/trunk/applications/NXsas.nxdl.xml&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Ron Ghosh has laid out details of a proposal to use HDF5/Nexus : [[HDF5 Notes Ghosh]]&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Peter Boesecke misses definitions of parameters that are needed to describe small-angle and wide-angle scattering experiments. Parameters like &amp;quot;Distance&amp;quot;, &amp;quot;Center&amp;quot;, &amp;quot;Rotation&amp;quot; have only a meaning when they are part of a geometrical model, otherwise they are useless. He has collected parameters that are required for SAS/WAS experiments with position sensitive detectors (1D and 2D). When saving experimental data it should be checked that these parameters are either implicitly or explicitly described by the supplied metadata: [[User:Boesecke | SX_parametrization]].&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
== Discussion ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category: canSAS 2012]]&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=930</id>
		<title>2012 Data Discussion</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=930"/>
		<updated>2012-07-19T09:24:51Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;*The following is the agenda of work posted under business for [[canSAS-2012]].  Please add comments here:&lt;br /&gt;
** &#039;&#039;&#039;1D Format&#039;&#039;&#039;&lt;br /&gt;
** agree a proposed foreign namespace extension of the current 1D standard (required to enable, for example, t-o-f instruments to store auxillary wavelength-dependent non-I(Q) data in the same output files)&lt;br /&gt;
*** see Section 1.6.5 in [http://svn.smallangles.net/trac/canSAS/browser/1dwg/tags/v1.0/doc/cansas-1d-1_0-manual.pdf?format=raw here]&lt;br /&gt;
*** and look at this [http://svn.smallangles.net/trac/canSAS/browser/1dwg/data/Glassy%20Carbon/ISIS/GLASSYC_C4G8G9_withTL.xml example]&lt;br /&gt;
*** or [http://www.smallangles.net/wgwiki/images/f/f5/ISIS_SASXML_v1_1_Monitor_Spectrum_Example.XML this] one&lt;br /&gt;
** agree resultant changes to the schema/stylesheet&lt;br /&gt;
    SMK  - For clarity, this extension was proposed &#039;&#039;after&#039;&#039; adoption of the existing version of the standard. Ratification of&lt;br /&gt;
           this extension at CanSAS-2012 would give facilities/software developers the necessary confidence to implement it.&lt;br /&gt;
    SMK  - This proposed extension would allow more-or-less any non-I(Q) data to be included in a CanSAS-1D data file under a&lt;br /&gt;
           suitable foreign namespace. That is remarkable flexibility, and it does not require any significant revision&lt;br /&gt;
           of the existing standard. However, it could be argued that certain types of non-I(Q) data are so integral to a SAS&lt;br /&gt;
           experiment that they should instead be given explicit SASXML tags within the standard? Transmission data is a good&lt;br /&gt;
           example of this: the existing standard explicitly includes a tag for the transmission value from a &#039;&#039;monochromatic&#039;&#039;&lt;br /&gt;
           measurement (SASsample\transmission) but makes no provision for transmission values from &#039;&#039;white beam&#039;&#039;&lt;br /&gt;
           measurements. The proposed foreign namespace extension will make such provision possible &#039;&#039;but only&#039;&#039; as an&lt;br /&gt;
           extension, not as a formal part of the standard. Is that acceptable? The downside of explicitly adding new SASXML&lt;br /&gt;
           tags to the existing standard is that it would require issuing a new version of the standard. &lt;br /&gt;
    ARJN - I would recommend that during this meeting that the current format then be &#039;parked&#039;, the new 2D format&lt;br /&gt;
           should be flexible enough to handle 1D and 2D data.&lt;br /&gt;
    SMK  - Agreed.&lt;br /&gt;
    ARR  - Perhaps we should be cautious about suggesting no further development for the existing 1-D format. Unless&lt;br /&gt;
           there is scope for adapting to future needs, it will be seen as not suitable for new uses.  This, of course,&lt;br /&gt;
           does not imply that there have to be active plans for further changes at present. &lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
** &#039;&#039;&#039;2D Format&#039;&#039;&#039;&lt;br /&gt;
** define minimum necessary for reduced data&lt;br /&gt;
*** review previous discussions on 2D&lt;br /&gt;
*** considerations specific to 2D reduced data&lt;br /&gt;
*** consider forward looking issues such as &lt;br /&gt;
**** grazing incidence&lt;br /&gt;
**** event mode analysis&lt;br /&gt;
** suggest format framework (NeXus extension, canSAS 1D extension, other) with brief discussion of the reason for the choice (including options considered, pros and cons of each, and final weighing)&lt;br /&gt;
*** compare with NeXus definitions for:&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas &#039;&#039;&#039;NXsas&#039;&#039;&#039;]&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXiqproc &#039;&#039;&#039;NXiqproc&#039;&#039;&#039;]&lt;br /&gt;
** Guide to how to make implementation easy.&lt;br /&gt;
** Create straw format suitable for test/demonstration use and convert some test data for such a demonstration.&lt;br /&gt;
** Provide a plan for presentation at SAS 2012&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
* A proposal for a 2D version of the canSAS 1D data format has been posted for discussion: [[2D Data Format Proposal]]&lt;br /&gt;
* NeXus has a definition for multi-dimensional data:&lt;br /&gt;
** http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas&lt;br /&gt;
** http://svn.nexusformat.org/definitions/trunk/applications/NXsas.nxdl.xml&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Ron Ghosh has laid out details of a proposal to use HDF5/Nexus : [[HDF5 Notes Ghosh]]&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Peter Boesecke misses definitions of parameters that are needed to describe small-angle and wide-angle scattering experiments. Parameters like &amp;quot;Distance&amp;quot;, &amp;quot;Center&amp;quot;, &amp;quot;Rotation&amp;quot; have only a meaning when they are part of a geometrical model, otherwise they are useless. He has collected parameters that are required for SAS/WAS experiments with position sensitive detectors (1D and 2D). When saving experimental data it should be checked that these parameters are either implicitly or explicitly described by metadata: [[User:Boesecke | SX_parametrization]].&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
== Discussion ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category: canSAS 2012]]&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=929</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=929"/>
		<updated>2012-07-19T09:17:33Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described SX-parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? It is surely not desirable to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX-parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
In addition to describe a given experimental geometry it should be possible to save experimental conditions (&#039;&#039;sample name&#039;&#039;, &#039;&#039;temperature&#039;&#039;, &#039;&#039;pressure&#039;&#039; etc.) and to have the possibility look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors. The geometrical description of SANS data should converge with the description of SAXS data for gravity -&amp;gt; 0 (just a wish).&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=928</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=928"/>
		<updated>2012-07-19T09:12:35Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described SX-parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? It is surely not desirable to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX-parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
In addition to describe a given experimental geometry it should be possible to save experimental conditions (&#039;&#039;sample name&#039;&#039;, &#039;&#039;temperature&#039;&#039;, &#039;&#039;pressure&#039;&#039; etc.) and to have the possibility look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=927</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=927"/>
		<updated>2012-07-19T09:11:36Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described SX-parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? It is surely not desirable to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX-parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
In addition to describe a given experimental geometry it should be possible to save experimental conditions (&#039;&#039;sample name&#039;&#039;, &#039;&#039;temperature&#039;&#039;, &#039;&#039;pressure&#039;&#039; etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=926</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=926"/>
		<updated>2012-07-19T09:10:59Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described SX-parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? It is surely not desirable to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX-parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
In addition to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=925</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=925"/>
		<updated>2012-07-19T09:10:14Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described SX-parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? It is surely not desirable to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX-parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=924</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=924"/>
		<updated>2012-07-19T09:08:53Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described SX-parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX-parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=923</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=923"/>
		<updated>2012-07-19T09:08:15Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to save all &#039;&#039;SX parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=922</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=922"/>
		<updated>2012-07-19T09:07:50Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. It would be sufficient to write either all &#039;&#039;SX parameters&#039;&#039; or a SAS file standard parameter list that contains them, at least implicitly.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=921</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=921"/>
		<updated>2012-07-19T09:04:33Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It becomes necessary to distinguish clearly between &#039;&#039;beam center&#039;&#039; and &#039;&#039;point of normal incidence&#039;&#039;. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=920</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=920"/>
		<updated>2012-07-19T09:03:19Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: &#039;&#039;pixel size&#039;&#039; in each direction, &#039;&#039;wavelength&#039;&#039;, &#039;&#039;distance&#039;&#039;, &#039;&#039;beam center&#039;&#039;). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=919</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=919"/>
		<updated>2012-07-19T09:01:50Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength and beam center.&lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=918</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=918"/>
		<updated>2012-07-19T08:58:03Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength. &lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. Linear and area detectors should be limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=917</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=917"/>
		<updated>2012-07-19T08:57:22Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength. &lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement, e.g. in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. In this sense linear and area detectors are limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=916</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=916"/>
		<updated>2012-07-19T08:56:48Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength. &lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a SAS file independent of its format (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. In this sense linear and area detectors are limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=915</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=915"/>
		<updated>2012-07-19T08:55:58Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength. &lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all listed parameters. But, whenever possible, I prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;br /&gt;
&lt;br /&gt;
The above description is suitable for pinhole type experiments with linear and area detectors. Other detector types or different experimental configurations may need additional information. Whenever possible the descriptions should converge for limiting cases, e.g. the description of cylindrical detector geometry should converge to the description of linear detector geometry when the cylindrical radius approaches infinity. In this sense linear and area detectors are limiting cases of cylindrical and spherical detectors.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=914</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=914"/>
		<updated>2012-07-19T08:34:35Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that the parameters do not become contradictory and that they remain well-defined. Many metadata parameters are not needed very often, e.g. proposal number, but some others are, e.g. wavelength. &lt;br /&gt;
&lt;br /&gt;
As internal reference a standard geometry of a small angle scattering experiment has been chosen where the position sensitive detector (1D or 2D) is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=913</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=913"/>
		<updated>2012-07-19T08:28:30Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Go back to [[2012_Data_Discussion]]&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and that it remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The chosen standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=912</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=912"/>
		<updated>2012-07-19T08:27:09Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and that it remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The chosen standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
*Description: &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=911</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=911"/>
		<updated>2012-07-19T08:26:39Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and that it remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The chosen standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | SX parametrization-ref-short]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=910</id>
		<title>2012 Data Discussion</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=910"/>
		<updated>2012-07-19T08:25:37Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;*The following is the agenda of work posted under business for [[canSAS-2012]].  Please add comments here:&lt;br /&gt;
** &#039;&#039;&#039;1D Format&#039;&#039;&#039;&lt;br /&gt;
** agree a proposed foreign namespace extension of the current 1D standard (required to enable, for example, t-o-f instruments to store auxillary wavelength-dependent non-I(Q) data in the same output files)&lt;br /&gt;
*** see Section 1.6.5 in [http://svn.smallangles.net/trac/canSAS/browser/1dwg/tags/v1.0/doc/cansas-1d-1_0-manual.pdf?format=raw here]&lt;br /&gt;
*** and look at this [http://svn.smallangles.net/trac/canSAS/browser/1dwg/data/Glassy%20Carbon/ISIS/GLASSYC_C4G8G9_withTL.xml example]&lt;br /&gt;
*** or [http://www.smallangles.net/wgwiki/images/f/f5/ISIS_SASXML_v1_1_Monitor_Spectrum_Example.XML this] one&lt;br /&gt;
** agree resultant changes to the schema/stylesheet&lt;br /&gt;
    SMK  - For clarity, this extension was proposed &#039;&#039;after&#039;&#039; adoption of the existing version of the standard. Ratification of&lt;br /&gt;
           this extension at CanSAS-2012 would give facilities/software developers the necessary confidence to implement it.&lt;br /&gt;
    SMK  - This proposed extension would allow more-or-less any non-I(Q) data to be included in a CanSAS-1D data file under a&lt;br /&gt;
           suitable foreign namespace. That is remarkable flexibility, and it does not require any significant revision&lt;br /&gt;
           of the existing standard. However, it could be argued that certain types of non-I(Q) data are so integral to a SAS&lt;br /&gt;
           experiment that they should instead be given explicit SASXML tags within the standard? Transmission data is a good&lt;br /&gt;
           example of this: the existing standard explicitly includes a tag for the transmission value from a &#039;&#039;monochromatic&#039;&#039;&lt;br /&gt;
           measurement (SASsample\transmission) but makes no provision for transmission values from &#039;&#039;white beam&#039;&#039;&lt;br /&gt;
           measurements. The proposed foreign namespace extension will make such provision possible &#039;&#039;but only&#039;&#039; as an&lt;br /&gt;
           extension, not as a formal part of the standard. Is that acceptable? The downside of explicitly adding new SASXML&lt;br /&gt;
           tags to the existing standard is that it would require issuing a new version of the standard. &lt;br /&gt;
    ARJN - I would recommend that during this meeting that the current format then be &#039;parked&#039;, the new 2D format&lt;br /&gt;
           should be flexible enough to handle 1D and 2D data.&lt;br /&gt;
    SMK  - Agreed.&lt;br /&gt;
    ARR  - Perhaps we should be cautious about suggesting no further development for the existing 1-D format. Unless&lt;br /&gt;
           there is scope for adapting to future needs, it will be seen as not suitable for new uses.  This, of course,&lt;br /&gt;
           does not imply that there have to be active plans for further changes at present. &lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
** &#039;&#039;&#039;2D Format&#039;&#039;&#039;&lt;br /&gt;
** define minimum necessary for reduced data&lt;br /&gt;
*** review previous discussions on 2D&lt;br /&gt;
*** considerations specific to 2D reduced data&lt;br /&gt;
*** consider forward looking issues such as &lt;br /&gt;
**** grazing incidence&lt;br /&gt;
**** event mode analysis&lt;br /&gt;
** suggest format framework (NeXus extension, canSAS 1D extension, other) with brief discussion of the reason for the choice (including options considered, pros and cons of each, and final weighing)&lt;br /&gt;
*** compare with NeXus definitions for:&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas &#039;&#039;&#039;NXsas&#039;&#039;&#039;]&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXiqproc &#039;&#039;&#039;NXiqproc&#039;&#039;&#039;]&lt;br /&gt;
** Guide to how to make implementation easy.&lt;br /&gt;
** Create straw format suitable for test/demonstration use and convert some test data for such a demonstration.&lt;br /&gt;
** Provide a plan for presentation at SAS 2012&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
* A proposal for a 2D version of the canSAS 1D data format has been posted for discussion: [[2D Data Format Proposal]]&lt;br /&gt;
* NeXus has a definition for multi-dimensional data:&lt;br /&gt;
** http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas&lt;br /&gt;
** http://svn.nexusformat.org/definitions/trunk/applications/NXsas.nxdl.xml&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Ron Ghosh has laid out details of a proposal to use HDF5/Nexus : [[HDF5 Notes Ghosh]]&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Peter Boesecke misses definitions of parameters that are needed to describe small-angle and wide-angle scattering experiments. Parameters like &amp;quot;Distance&amp;quot; have only a unique meaning when they are part of a specific geometrical model, otherwise they are useless. He has collected parameters that are required for SAS/WAS experiments with position sensitive detectors (1D and 2D). When saving experimental data it should be checked that these parameters are either implicitly or explicitly described by metadata: [[User:Boesecke | SX_parametrization]].&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
== Discussion ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category: canSAS 2012]]&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=909</id>
		<title>2012 Data Discussion</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=2012_Data_Discussion&amp;diff=909"/>
		<updated>2012-07-19T08:24:03Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;*The following is the agenda of work posted under business for [[canSAS-2012]].  Please add comments here:&lt;br /&gt;
** &#039;&#039;&#039;1D Format&#039;&#039;&#039;&lt;br /&gt;
** agree a proposed foreign namespace extension of the current 1D standard (required to enable, for example, t-o-f instruments to store auxillary wavelength-dependent non-I(Q) data in the same output files)&lt;br /&gt;
*** see Section 1.6.5 in [http://svn.smallangles.net/trac/canSAS/browser/1dwg/tags/v1.0/doc/cansas-1d-1_0-manual.pdf?format=raw here]&lt;br /&gt;
*** and look at this [http://svn.smallangles.net/trac/canSAS/browser/1dwg/data/Glassy%20Carbon/ISIS/GLASSYC_C4G8G9_withTL.xml example]&lt;br /&gt;
*** or [http://www.smallangles.net/wgwiki/images/f/f5/ISIS_SASXML_v1_1_Monitor_Spectrum_Example.XML this] one&lt;br /&gt;
** agree resultant changes to the schema/stylesheet&lt;br /&gt;
    SMK  - For clarity, this extension was proposed &#039;&#039;after&#039;&#039; adoption of the existing version of the standard. Ratification of&lt;br /&gt;
           this extension at CanSAS-2012 would give facilities/software developers the necessary confidence to implement it.&lt;br /&gt;
    SMK  - This proposed extension would allow more-or-less any non-I(Q) data to be included in a CanSAS-1D data file under a&lt;br /&gt;
           suitable foreign namespace. That is remarkable flexibility, and it does not require any significant revision&lt;br /&gt;
           of the existing standard. However, it could be argued that certain types of non-I(Q) data are so integral to a SAS&lt;br /&gt;
           experiment that they should instead be given explicit SASXML tags within the standard? Transmission data is a good&lt;br /&gt;
           example of this: the existing standard explicitly includes a tag for the transmission value from a &#039;&#039;monochromatic&#039;&#039;&lt;br /&gt;
           measurement (SASsample\transmission) but makes no provision for transmission values from &#039;&#039;white beam&#039;&#039;&lt;br /&gt;
           measurements. The proposed foreign namespace extension will make such provision possible &#039;&#039;but only&#039;&#039; as an&lt;br /&gt;
           extension, not as a formal part of the standard. Is that acceptable? The downside of explicitly adding new SASXML&lt;br /&gt;
           tags to the existing standard is that it would require issuing a new version of the standard. &lt;br /&gt;
    ARJN - I would recommend that during this meeting that the current format then be &#039;parked&#039;, the new 2D format&lt;br /&gt;
           should be flexible enough to handle 1D and 2D data.&lt;br /&gt;
    SMK  - Agreed.&lt;br /&gt;
    ARR  - Perhaps we should be cautious about suggesting no further development for the existing 1-D format. Unless&lt;br /&gt;
           there is scope for adapting to future needs, it will be seen as not suitable for new uses.  This, of course,&lt;br /&gt;
           does not imply that there have to be active plans for further changes at present. &lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
** &#039;&#039;&#039;2D Format&#039;&#039;&#039;&lt;br /&gt;
** define minimum necessary for reduced data&lt;br /&gt;
*** review previous discussions on 2D&lt;br /&gt;
*** considerations specific to 2D reduced data&lt;br /&gt;
*** consider forward looking issues such as &lt;br /&gt;
**** grazing incidence&lt;br /&gt;
**** event mode analysis&lt;br /&gt;
** suggest format framework (NeXus extension, canSAS 1D extension, other) with brief discussion of the reason for the choice (including options considered, pros and cons of each, and final weighing)&lt;br /&gt;
*** compare with NeXus definitions for:&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas &#039;&#039;&#039;NXsas&#039;&#039;&#039;]&lt;br /&gt;
**** [http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXiqproc &#039;&#039;&#039;NXiqproc&#039;&#039;&#039;]&lt;br /&gt;
** Guide to how to make implementation easy.&lt;br /&gt;
** Create straw format suitable for test/demonstration use and convert some test data for such a demonstration.&lt;br /&gt;
** Provide a plan for presentation at SAS 2012&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
* A proposal for a 2D version of the canSAS 1D data format has been posted for discussion: [[2D Data Format Proposal]]&lt;br /&gt;
* NeXus has a definition for multi-dimensional data:&lt;br /&gt;
** http://download.nexusformat.org/doc/html/ClassDefinitions-Application.html#NXsas&lt;br /&gt;
** http://svn.nexusformat.org/definitions/trunk/applications/NXsas.nxdl.xml&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Ron Ghosh has laid out details of a proposal to use HDF5/Nexus : [[HDF5 Notes Ghosh]]&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
* Peter Boesecke misses definitions of parameters that are needed to describe small-angle and wide-angle scattering experiments. Parameters like &amp;quot;Distance&amp;quot; have only a unique meaning when they are part of a specific geometrical model, otherwise they are useless. He has collected parameters that are required for SAS/WAS experiments with position sensitive detectors (1D and 2D). When saving experimental data it should be checked that these parameters are either implicitly or explicitly described by metadata: [[User:Boesecke]].&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
== Discussion ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category: canSAS 2012]]&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=908</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=908"/>
		<updated>2012-07-18T17:29:19Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and that it remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The chosen standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). The use of regions of interest and binning must be supported without complicated recalibration. It should be possible to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm. &lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=907</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=907"/>
		<updated>2012-07-18T17:26:33Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and that it remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). I need to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=906</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=906"/>
		<updated>2012-07-18T17:23:24Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). I need to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke, &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=905</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=905"/>
		<updated>2012-07-18T17:23:08Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. The parameter set was evolving with time and I have tried to make sure that it does not become contradictory and remains well-defined. Many metadata parameters are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). I need to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose to store, optionally, the variance of each pixel (see: Peter Boesecke 􀀀 &amp;quot;Reduction of scattering data&amp;quot; J. Appl. Cryst. (2007). 40, s423–s427)&lt;br /&gt;
&lt;br /&gt;
Additionally to describe a given experimental geometry it should be possible to save experimental conditions (temperature, pressure etc.) in a defined way and to look-up experiments in a data base. But this is out of the scope of this contribution.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=904</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=904"/>
		<updated>2012-07-18T17:11:53Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. &lt;br /&gt;
&lt;br /&gt;
The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel size in each direction, wavelength, distance, beam center). I need to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. Therefore, parameters are added that default to the standard case when not specified. An inclined detector is described by additional rotation angles that are zero when not defined. It is now also necessary to distinguish the beam center and the point of normal incidence. Sometimes it can also become more comfortable to look to the data in a different way, e.g. to construct a physical detector mask. In this case distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=903</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=903"/>
		<updated>2012-07-18T17:06:25Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: &#039;&#039;What data must be saved, what data are needed for analysis?&#039;&#039; As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel sizes, wavelength, distance, beam center). I want to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. I add parameters that default to the standard case when not given. An inclined detector is described by additional rotation angles that are zero when not defined. It can also be necessary to look to the data in a different way, e.g. to construct a physical detector mask, where distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=902</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=902"/>
		<updated>2012-07-18T17:05:40Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: What data must be saved, what data are needed for analysis? As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel sizes, wavelength, distance, beam center). I want to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. I add parameters that default to the standard case when not given. An inclined detector is described by additional rotation angles that are zero when not defined. It can also be necessary to look to the data in a different way, e.g. to construct a physical detector mask, where distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown &#039;&#039;&#039;[[media:SX parametrization-ref-short 20120217.pdf | here]]&#039;&#039;&#039;. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (task: what are the corresponding NEXUS parameters?). How could/must they be saved after refinement in a standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my parameters. But, whenever possible, I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=901</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=901"/>
		<updated>2012-07-18T17:04:03Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: What data must be saved, what data are needed for analysis? As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel sizes, wavelength, distance, beam center). I want to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. I add parameters that default to the standard case when not given. An inclined detector is described by additional rotation angles that are zero when not defined. It can also be necessary to look to the data in a different way, e.g. to construct a physical detector mask, where distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of this parametrization it is shown [[media:SX parametrization-ref-short 20120217.pdf | here]]. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (what are the corresponding NEXUS parameters?). How could/must I save them after refinement in the standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my own parameters. But I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=900</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=900"/>
		<updated>2012-07-18T17:03:39Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: What data must be saved, what data are needed for analysis? As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel sizes, wavelength, distance, beam center). I want to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. I add parameters that default to the standard case when not given. An inclined detector is described by additional rotation angles that are zero when not defined. It can also be necessary to look to the data in a different way, e.g. to construct a physical detector mask, where distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of my parametrization it is shown [[media:SX parametrization-ref-short 20120217.pdf | here]]. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (what are the corresponding NEXUS parameters?). How could/must I save them after refinement in the standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my own parameters. But I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=899</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=899"/>
		<updated>2012-07-18T17:03:18Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: What data must be saved, what data are needed for analysis? As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel sizes, wavelength, distance, beam center). I want to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. I add parameters that default to the standard case when not given. An inclined detector is described by additional rotation angles that are zero when not defined. It can also be necessary to look to the data in a different way, e.g. to construct a physical detector mask, where distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of my parametrization it is shown [[SX parametrization-ref-short 20120217.pdf | here]]. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (what are the corresponding NEXUS parameters?). How could/must I save them after refinement in the standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my own parameters. But I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=File:SX_parametrization-ref-short_20120217.pdf&amp;diff=898</id>
		<title>File:SX parametrization-ref-short 20120217.pdf</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=File:SX_parametrization-ref-short_20120217.pdf&amp;diff=898"/>
		<updated>2012-07-18T17:02:42Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
	<entry>
		<id>https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=897</id>
		<title>User:Boesecke</title>
		<link rel="alternate" type="text/html" href="https://wiki.cansas.org/index.php?title=User:Boesecke&amp;diff=897"/>
		<updated>2012-07-18T17:01:04Z</updated>

		<summary type="html">&lt;p&gt;Boesecke: Created page with &amp;quot;from Peter Boesecke (ESRF, Grenoble)  The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am ...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;from Peter Boesecke (ESRF, Grenoble)&lt;br /&gt;
&lt;br /&gt;
The discussion in what format small angle scattering data should be saved is already going on for many years: XML, HDF5, NEXUS etc. I am convinced that this is not the most important question that must be answered. If somebody would decide: &amp;quot;It is BXHN&amp;quot; (just a name) I would not feel better because the most important part would still be missing: What data must be saved, what data are needed for analysis? As beamline scientist and local contact at X-ray scattering beamlines I have always tried to save as much useful metadata as possible together with the (2D) scattering data. I have always tried to make sure that the used geometrical parameters are not contradictory, i.e. well-defined. Many of these metadata are not needed very often, e.g. the proposal number, but some are practically always needed, e.g. the wavelength. The standard geometry is a small angle scattering experiment where the (1D, 2D) detector is perpendicular to the primary beam (required metadata: pixel sizes, wavelength, distance, beam center). I want to be able to analyze in a similar way standard geometry data and data from more complicated geometries, e.g. inclined detectors. I add parameters that default to the standard case when not given. An inclined detector is described by additional rotation angles that are zero when not defined. It can also be necessary to look to the data in a different way, e.g. to construct a physical detector mask, where distances in mm are much more adequate than in 1/nm.&lt;br /&gt;
&lt;br /&gt;
A description of my parametrization it is shown here. &lt;br /&gt;
&lt;br /&gt;
It must be possible to extract the described parameters from a standard SAS file (what are the corresponding NEXUS parameters?). How could/must I save them after refinement in the standard SAS file? I surely do not want to overwrite any raw data, e.g. the monochromator rotation. For me it would be sufficient to write all my own parameters. But I would prefer a common way.&lt;br /&gt;
&lt;br /&gt;
For statistical error propagation calculations I propose the optional use of a variance array that contains the variance of each pixel.&lt;/div&gt;</summary>
		<author><name>Boesecke</name></author>
	</entry>
</feed>