Changeset 64eecf7 in sasmodels for doc/guide/magnetism

Timestamp:

Sep 5, 2017 11:40:09 AM (7 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:

30b60d2

Parents:

a53bf6b (diff), 142a8e2 (diff)
Note: this is a merge changeset, the changes displayed below correspond to the merge itself.
Use the (diff) links above to see all the changes relative to each parent.

Message:

Merge branch 'master' into ticket-510

Location:

doc/guide/magnetism

Files:

• mag_img/M_angles_pic.png (moved) (moved from doc/ref/magnetism/mag_img/M_angles_pic.png)
• magnetism.rst (moved) (moved from doc/ref/magnetism/magnetism.rst) (2 diffs)
• mag_img/M_angles_pic.bmp (deleted)
• mag_img/mag_vector.bmp (deleted)

doc/guide/magnetism/magnetism.rst

@@ -2 +2 @@
 
 Polarisation/Magnetic Scattering
-=======================================================
+================================
 
-In earlier versions of SasView magnetic scattering was implemented in just five 
-(2D) models
-
-*  :ref:`sphere`
-*  :ref:`core-shell-sphere`
-*  :ref:`core-multi-shell`
-*  :ref:`cylinder`
-*  :ref:`parallelepiped`
-
-From SasView 4.x it is implemented on most models in the 'shape' category.
-
-In general, the scattering length density (SLD = $\beta$) in each region where the
-SLD is uniform, is a combination of the nuclear and magnetic SLDs and, for polarised
-neutrons, also depends on the spin states of the neutrons.
+Models which define a scattering length density parameter can be evaluated
+ as magnetic models. In general, the scattering length density (SLD =
+ $\beta$) in each region where the SLD is uniform, is a combination of the
+ nuclear and magnetic SLDs and, for polarised neutrons, also depends on the
+ spin states of the neutrons.
 
 For magnetic scattering, only the magnetization component $\mathbf{M_\perp}$
@@ -98 +89 @@
 .. note::
     This help document was last changed by Steve King, 02May2015
+
+* Document History *
+
+| 2017-05-08 Paul Kienzle