ESS_GUIESS_GUI_DocsESS_GUI_batch_fittingESS_GUI_bumps_abstractionESS_GUI_iss1116ESS_GUI_iss879ESS_GUI_iss959ESS_GUI_openclESS_GUI_orderingESS_GUI_sync_sascalccostrafo411magnetic_scattrelease-4.1.1release-4.1.2release-4.2.2release_4.0.1ticket-1009ticket-1094-headlessticket-1242-2d-resolutionticket-1243ticket-1249ticket885unittest-saveload
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Last change
on this file since 17a6843 was
a55fac1,
checked in by Mathieu Doucet <doucetm@…>, 16 years ago
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Modified 2D non-shape models to be the same as 1D when not defined otherwise
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Property mode set to
100644
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File size:
1.7 KB
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| 1 | Release Notes |
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| 2 | ============= |
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| 3 | |
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| 4 | SANS Models version 0.4.1 |
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| 5 | |
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| 6 | Package name: sans.models |
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| 7 | |
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| 8 | 1- What's New in Version 0.4.1 |
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| 9 | - Release date: 6/9/2008 |
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| 10 | - Modified non-shape models so that the 2D output is the 1D output for the length of Q |
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| 11 | |
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| 12 | Version 0.4.0 |
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| 13 | - Release date: 4/15/2008 |
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| 14 | - Added shape-independent models. |
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| 15 | |
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| 16 | Version 0.3.2: |
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| 17 | - Release date: 2/14/2008 |
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| 18 | - Added models to be used in magnetic analysis. |
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| 19 | |
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| 20 | |
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| 21 | 2- Downloading and Installing |
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| 22 | |
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| 23 | 2.1- System Requirements: |
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| 24 | - Python version >= 2.4 should be running on the system |
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| 25 | |
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| 26 | 2.2- Installing: |
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| 27 | - Get the code from svn://danse.us/sans/releases/sansmodels-0.4.0 |
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| 28 | - Execute the following: |
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| 29 | python setup.py install |
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| 30 | |
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| 31 | 3- Known Issues |
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| 32 | |
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| 33 | 3.1- All systems: |
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| 34 | - Q range validity of I(q) calculations. |
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| 35 | Our 1D models of I(q) use the function of the NCNR library |
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| 36 | for their IGOR package (Klein, 2006). That library uses a |
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| 37 | fsat integration technique in some of its models (cylinders |
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| 38 | and ellipsoids). Integration is done using 76 points in the |
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| 39 | angle between the axis of the object and the q-vector, which |
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| 40 | translates in a larger inaccuracy at high q. Integratiing |
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| 41 | the 2D model I(q,phi) over all orientations of the object |
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| 42 | will not yield the exact same result as the NCNR calculation |
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| 43 | for q > 0.3 A-1. |
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| 44 | |
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| 45 | 3.2- Windows: |
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| 46 | - None |
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| 47 | |
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| 48 | 3.3- Linux: |
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| 49 | - None |
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| 50 | |
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| 51 | 4- Troubleshooting |
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| 52 | |
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| 53 | - None |
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| 54 | |
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| 55 | 5- Frequently Asked Questions |
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| 56 | |
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| 57 | - None |
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| 58 | |
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| 59 | 6- Other Resources |
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| 60 | |
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| 61 | - See: http://danse.us/trac/sans/wiki/8_2_2_1DModelFitting |
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| 62 | - See: http://danse.us/trac/sans/wiki/8_2_3_2DModeling |
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| 63 | - See: http://danse.us/trac/sans/wiki/8_2_6_model_extensions |
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| 64 | - See: http://danse.us/trac/sans/wiki/8_2_1Nonshape_models |
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| 65 | |
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| 66 | |
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| 67 | |
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| 68 | |
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| 69 | |
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| 70 | |
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