Changeset 8ae8532 in sasmodels for doc/guide


Ignore:
Timestamp:
May 7, 2017 4:24:16 PM (8 years ago)
Author:
Paul Kienzle <pkienzle@…>
Branches:
master, core_shell_microgels, costrafo411, magnetic_model, ticket-1257-vesicle-product, ticket_1156, ticket_1265_superball, ticket_822_more_unit_tests
Children:
990d8df
Parents:
630156b
Message:

doc reorg

Location:
doc/guide
Files:
2 added
1 edited
10 moved

Legend:

Unmodified
Added
Removed

  • doc/guide/gpu/gpu_computations.rst

    r3f5a566 r8ae8532  
    44GPU Computations 
    55**************** 
    6 SasView model evaluations can run on your graphics card (GPU) or they can run 
     6sasmodels evaluations can run on your graphics card (GPU) or they can run 
    77on the processor (CPU). In general, calculations performed on the GPU will run faster. 
    88 
    … …  
    3232 
    3333SasView prefers AMD or NVIDIA drivers for GPU, and prefers Intel or 
    34 Apple drivers for CPU. Both GPU and CPU are included on the assumption that CPU  
     34Apple drivers for CPU. Both GPU and CPU are included on the assumption that CPU 
    3535is always available and supports double precision. 
    3636 
    … …  
    6363 
    6464 
    65 .. note:: 
    66     This help document was last changed by Steve King, 08Oct2016 
     65*Document History* 
     66 
     67| 2016-10-08 Steve King 
     68| 2017-05-07 Paul Kienzle 

  • doc/guide/index.rst

    rbb6f0f3 r8ae8532  
    1 ********** 
    2 SAS Models 
    3 ********** 
     1**************** 
     2SAS Models Guide 
     3**************** 
    44 
    5 Small angle X-ray and Neutron (SAXS and SANS) scattering examines the 
    6 scattering patterns produced by a beam travelling through the sample 
    7 and scattering at low angles.  The scattering is computed as a function 
    8 of $q_x$ and $q_y$, which for a given beam wavelength corresponds to 
    9 particular scattering angles. Each pixel on the detector corresponds to 
    10 a different scattering angle. If the sample is unoriented, the scattering 
    11 pattern will appear as rings on the detector.  In this case, a circular 
    12 average can be taken with 1-dimension data at $q = \surd (q_x^2 + q_y^2)$ 
    13 compared to the orientationally averaged SAS scattering pattern. 
     5.. toctree:: 
     6   :numbered: 4 
     7   :maxdepth: 4 
    148 
    15 Models have certain features in common. 
    16  
    17 Every model has a *scale* and a *background*. 
    18  
    19 Talk about orientation, with diagrams for orientation so that we don't need 
    20 a link on every model page? 
    21  
    22 .. _orientation: 
    23  
    24 .. figure: img/orientation1.jpg 
    25  
    26     Orientation in 3D 
    27  
    28 .. figure: img/orientation2.jpg 
    29  
    30     Orientation cross sections 
    31  
    32 Talk about polydispersity. 
    33  
    34 Talk about magnetism, converting the magnetism help file to inline text here, 
    35 with links so that models can point back to it. 
    36  
    37 Need to talk about structure factors even though we don't have any 
    38 implemented yet. 
     9   intro.rst 
     10   gpu/gpu_computations.rst 
     11   gpu/opencl_installation.rst 
     12   magnetism/magnetism.rst 
     13   sesans/sans_to_sesans.rst 
     14   sesans/sesans_fitting.rst 
     15   refs.rst 

  • doc/guide/sesans/sesans_fitting.rst

    r3330bb4 r8ae8532  
    77=================== 
    88 
    9 .. note:: A proper installation of the developers setup of SasView (http://trac.sasview.org/wiki/AnacondaSetup) is a prerequisite for using these instructions. 
     9.. note:: 
     10 
     11    A proper installation of the developers setup of SasView 
     12    (http://trac.sasview.org/wiki/AnacondaSetup) is a prerequisite for 
     13    using these instructions. 
    1014 
    1115It is possible to fit SESANS measurements from the command line in Python. 
    … …  
    1317Simple Fits 
    1418........... 
    15 In the folder sasmodels/example the file sesans_sphere_2micron.py gives an example of how to fit a shape to a measurement. 
     19In the folder sasmodels/example the file sesans_sphere_2micron.py gives 
     20an example of how to fit a shape to a measurement. 
    1621 
    1722The command:: 
    … …  
    2328.. image:: sesans_img/SphereLineFitSasView.png 
    2429 
    25 All the parameters and names in sesans_sphere_2micron.py (shown below) can be adjusted to fit your own problem:: 
     30All the parameters and names in sesans_sphere_2micron.py (shown below) can 
     31be adjusted to fit your own problem:: 
    2632 
    2733  """ 
    … …  
    6470  # Constraints 
    6571  # model.param_name = f(other params) 
    66   # EXAMPLE: model.scale = model.radius*model.radius*(1 - phi) - where radius and scale are model functions and phi is 
    67   # a custom parameter 
     72  # EXAMPLE: model.scale = model.radius*model.radius*(1 - phi) - where radius 
     73  # and scale are model functions and phi is a custom parameter 
    6874  model.scale = phi*(1-phi) 
    6975 
    … …  
    7480Incorporating a Structure Factor 
    7581................................ 
    76 An example of how to also include a structure factor can be seen in the following example taken from Washington et al.,  
    77 *Soft Matter*\, (2014), 10, 3016 (dx.doi.org/10.1039/C3SM53027B). These are time-of-flight measurements, which is the  
    78 reason that not the polarisation is plotted, but the :math:`\frac{log(P/P_0)}{\lambda^2}` . The sample is a dispersion  
    79 of core-shell colloids at a high volume fraction with hard sphere interactions. 
     82An example of how to also include a structure factor can be seen in the 
     83following example taken from Washington et al., *Soft Matter*\, (2014), 10, 3016 
     84(dx.doi.org/10.1039/C3SM53027B). These are time-of-flight measurements, which 
     85is the reason that not the polarisation is plotted, but the 
     86:math:`\frac{log(P/P_0)}{\lambda^2}` . The sample is a dispersion of 
     87core-shell colloids at a high volume fraction with hard sphere interactions. 
    8088 
    8189The fit can be started by:: 
    … …  
    8795.. image:: sesans_img/HardSphereLineFitSasView.png 
    8896 
    89 The code sesans_parameters_css-hs.py can then be used as a template for a fitting problem with a structure factor:: 
     97The code sesans_parameters_css-hs.py can then be used as a template for a 
     98fitting problem with a structure factor:: 
    9099 
    91100 """ 
    … …  
    131140 # Constraints 
    132141 # model.param_name = f(other params) 
    133  # EXAMPLE: model.scale = model.radius*model.radius*(1 - phi) - where radius and scale are model functions and phi is 
    134  # a custom parameter 
     142 # EXAMPLE: model.scale = model.radius*model.radius*(1 - phi) - where radius 
     143 # and scale are model functions and phi is a custom parameter 
    135144 model.scale = phi*(1-phi) 
    136145 model.volfraction = phi 
Note: See TracChangeset for help on using the changeset viewer.