- Timestamp:
- Oct 28, 2017 6:42:15 AM (7 years ago)
- Branches:
- master, core_shell_microgels, magnetic_model, ticket-1257-vesicle-product, ticket_1156, ticket_1265_superball, ticket_822_more_unit_tests
- Children:
- 5f8b72b
- Parents:
- da5536f
- Location:
- doc/guide
- Files:
-
- 2 edited
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doc/guide/orientation/orientation.rst
rda5536f reda8b30 42 42 cylinder cross section. (When $\theta = \phi = 0$ these are parallel to the $Y$ and $X$ axes of the instrument.) 43 43 The third orientation distribution, in $\psi$, is about the $c$ axis of the particle. Some experimentation may be required to 44 understand the 2d patterns fully. A number of different shapes of distribution are available, as described for polydispersity. 44 understand the 2d patterns fully. A number of different shapes of distribution are available, as described for 45 polydispersity, see :ref:`polydispersityhelp` . 45 46 46 47 Earlier versions of SasView had numerical integration issues in some circumstances when … … 52 53 values of Npts and Nsigs, the number of steps used in the integration and the range spanned in number of standard deviations. 53 54 The standard deviation is entered in units of degrees. For a rectangular (uniform) distribution the full width 54 should be $\pm\sqrt(3)$ ~ 1.73 standard deviations .55 should be $\pm\sqrt(3)$ ~ 1.73 standard deviations (this may be changed soon). 55 56 56 57 Where appropriate, for best numerical results, keep $a < b < c$ and the $\theta$ distribution narrower than the $\phi$ distribution. 57 58 58 Some more detailed technical notes are provided in the Developer section of this manual.59 Some more detailed technical notes are provided in the developer section of this manual :ref:`orientation_developer` . 59 60 60 61 *Document History* -
doc/guide/pd/polydispersity.rst
r1f058ea reda8b30 6 6 .. ZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZ 7 7 8 .. _polydispersityhelp: 9 8 10 Polydispersity Distributions 9 11 ---------------------------- 10 12 11 With some models in sasmodels we can calculate the average form factorfor a13 With some models in sasmodels we can calculate the average intensity for a 12 14 population of particles that exhibit size and/or orientational 13 polydispersity. The resultant form factoris normalized by the average15 polydispersity. The resultant intensity is normalized by the average 14 16 particle volume such that 15 17
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