source: sasview/docs/sphinx-docs/source/user/sasgui/perspectives/fitting/mag_help.rst @ 49148bb

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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[49148bb]1.. mag_help.rst
2
3.. This is a port of text from the original SasView html help file to ReSTructured text
4.. by S King, ISIS, during SasView CodeCamp-III in Feb 2015.
5
6.. |inlineimage004| image:: sm_image004.gif
7.. |inlineimage005| image:: sm_image005.gif
8.. |inlineimage008| image:: sm_image008.gif
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15
16
17.. ZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZ
18
19Polarisation/Magnetic Scattering
20--------------------------------
21
22Magnetic scattering is implemented in five (2D) models
23
24*  *SphereModel*
25*  *CoreShellModel*
26*  *CoreMultiShellModel*
27*  *CylinderModel*
28*  *ParallelepipedModel*
29
30In general, the scattering length density (SLD, = |beta|) in each region where the
31SLD is uniform, is a combination of the nuclear and magnetic SLDs and, for polarised
32neutrons, also depends on the spin states of the neutrons.
33
34For magnetic scattering, only the magnetization component, *M*\ :sub:`perp`,
35perpendicular to the scattering vector *Q* contributes to the the magnetic
36scattering length.
37
38.. image:: mag_vector.bmp
39
40The magnetic scattering length density is then
41
42.. image:: dm_eq.gif
43
44where |gamma| = -1.913 is the gyromagnetic ratio, |mu|\ :sub:`B` is the
45Bohr magneton, *r*\ :sub:`0` is the classical radius of electron, and |sigma|
46is the Pauli spin.
47
48Assuming that incident neutrons are polarized parallel (+) and anti-parallel (-)
49to the *x'* axis, the possible spin states after the sample are then
50
51No spin-flips (+ +) and (- -)
52
53Spin-flips    (+ -) and (- +)
54
55.. image:: M_angles_pic.bmp
56
57If the angles of the *Q* vector and the spin-axis (*x'*) to the *x*-axis are |phi|
58and |theta|\ :sub:`up`, respectively, then, depending on the spin state of the
59neutrons, the scattering length densities, including the nuclear scattering
60length density (|beta|\ :sub:`N`) are
61
62.. image:: sld1.gif
63
64when there are no spin-flips, and
65
66.. image:: sld2.gif
67
68when there are, and
69
70.. image:: mxp.gif
71
72.. image:: myp.gif
73
74.. image:: mzp.gif
75
76.. image:: mqx.gif
77
78.. image:: mqy.gif
79
80Here, *M*\ :sub:`0x`, *M*\ :sub:`0y` and *M*\ :sub:`0z` are the x, y and z components
81of the magnetization vector given in the laboratory xyz frame given by
82
83.. image:: m0x_eq.gif
84
85.. image:: m0y_eq.gif
86
87.. image:: m0z_eq.gif
88
89and the magnetization angles |theta|\ :sub:`M` and |phi|\ :sub:`M` are defined in
90the figure above.
91
92The user input parameters are:
93
94===========   ================================================================
95 M0_sld        = *D*\ :sub:`M` *M*\ :sub:`0`
96 Up_theta      = |theta|\ :sub:`up`
97 M_theta       = |theta|\ :sub:`M`
98 M_phi         = |phi|\ :sub:`M`
99 Up_frac_i     = (spin up)/(spin up + spin down) neutrons *before* the sample
100 Up_frac_f     = (spin up)/(spin up + spin down) neutrons *after* the sample
101===========   ================================================================
102
103*Note:* The values of the 'Up_frac_i' and 'Up_frac_f' must be in the range 0 to 1.
104
105.. ZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZ
106
107.. note::  This help document was last changed by Steve King, 02May2015
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