source: sasview/sansmodels/src/release_notes.txt @ b88c6e0

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
Last change on this file since b88c6e0 was b88c6e0, checked in by Mathieu Doucet <doucetm@…>, 16 years ago

Working on refactoring models (not done)

  • Property mode set to 100644
File size: 2.3 KB
Line 
1Release Notes
2=============
3
4SANS Models version 0.4.1
5
6Package name: sans.models
7
81- What's New in Version 0.?
9    - Release date: ?
10    - C extension models now use new C++ classes that incorporate dispersity and averaging
11      functionality.
12   
13    Version 0.4.1
14    - Release date: 6/9/2008
15    - Modified non-shape models so that the 2D output is the 1D output for the length of Q
16
17    Version 0.4.0
18        - Release date: 4/15/2008
19        - Added shape-independent models.
20       
21        Version 0.3.2:
22        - Release date: 2/14/2008
23        - Added models to be used in magnetic analysis.
24
25
262- Downloading and Installing
27
28        2.1- System Requirements:
29                - Python version >= 2.4 should be running on the system
30
31        2.2- Installing:
32                - Get the code from svn://danse.us/sans/releases/sansmodels-0.4.0
33                - Execute the following:
34                        python setup.py install
35
363- Known Issues
37
38        3.1- All systems:
39                - Q range validity of I(q) calculations.
40                        Our 1D models of I(q) use the function of the NCNR library
41                        for their IGOR package (Klein, 2006). That library uses a
42                        fsat integration technique in some of its models (cylinders
43                        and ellipsoids). Integration is done using 76 points in the
44                        angle between the axis of the object and the q-vector, which
45                        translates in a larger inaccuracy at high q. Integratiing
46                        the 2D model I(q,phi) over all orientations of the object
47                        will not yield the exact same result as the NCNR calculation
48                        for q > 0.3 A-1.
49                - Refactoring needs to be done to update the model base class.
50                  We should get rid of the useless arithmetics and store the parameters
51                  as class objects rather than values. This would eliminate the multitude
52                  of dictionaries needed to store all the various aspects of a parameter
53                  (limits, units, dispersity information). The C++ design it relies
54                  on is much cleaner in that respect, but it still depends on the old
55                  C computation. Those should be incorporated in the C++ classes.
56
57        3.2- Windows:
58                - None
59
60        3.3- Linux:
61                - None
62
634- Troubleshooting
64
65        - None
66
675- Frequently Asked Questions
68
69        - None
70
716- Other Resources
72
73        - See: http://danse.us/trac/sans/wiki/8_2_2_1DModelFitting
74        - See: http://danse.us/trac/sans/wiki/8_2_3_2DModeling
75        - See: http://danse.us/trac/sans/wiki/8_2_6_model_extensions
76        - See: http://danse.us/trac/sans/wiki/8_2_1Nonshape_models
77
78       
79
80       
81
82
Note: See TracBrowser for help on using the repository browser.