Changeset 906a325 in sasview

Timestamp:

Feb 27, 2015 10:24:44 PM (9 years ago)

Author:

butler

Branches:

master, ESS_GUI, ESS_GUI_Docs, ESS_GUI_batch_fitting, ESS_GUI_bumps_abstraction, ESS_GUI_iss1116, ESS_GUI_iss879, ESS_GUI_iss959, ESS_GUI_opencl, ESS_GUI_ordering, ESS_GUI_sync_sascalc, costrafo411, magnetic_scatt, release-4.1.1, release-4.1.2, release-4.2.2, release_4.0.1, ticket-1009, ticket-1094-headless, ticket-1242-2d-resolution, ticket-1243, ticket-1249, ticket885, unittest-saveload

Children:

cfe472e

Parents:

caf3baa6

Message:

Edited documentation to make clear that HPMSA model is the RMSA pursuant
to Karen Edler query. This is a common question according to Steve
Kline.

File:

• src/sas/models/media/model_functions.rst (modified) (1 diff)

src/sas/models/media/model_functions.rst

@@ -4800 +4800 @@
 **2.3.3. HayterMSAStructure Factor**
 
-This calculates the structure factor (the Fourier transform of the pair correlation function *g(r)*) for a system of
-charged, spheroidal objects in a dielectric medium. When combined with an appropriate form factor (such as sphere,
-core+shell, ellipsoid, etc), this allows for inclusion of the interparticle interference effects due to screened coulomb
-repulsion between charged particles.
+This is an implementation of the Rescaled Mean Spherical Approximation which calculates the structure factor (the 
+Fourier transform of the pair correlation function *g(r)*) for a system of charged, spheroidal objects in a
+dielectric medium. When combined with an appropriate form factor (such as sphere,core+shell, ellipsoid, etc), this
+allows for inclusion of the interparticle interference effects due to screened coulomb repulsion between charged particles.
 
 **This routine only works for charged particles**. If the charge is set to zero the routine will self-destruct!