source: sasmodels/doc/ref/sesans/sans_to_sesans.rst @ fac23b3

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[3330bb4]1.. currentmodule:: sasmodels
2.. Wim Bouwman, DUT, written at codecamp-V, Oct2016
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4.. _SESANS:
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6SANS to SESANS conversion
7=========================
8
9The conversion from SANS into SESANS in absolute units is a simple Hankel transformation when all the small-angle scattered neutrons are detected.
10First we calculate the Hankel transform including the absolute intensities by
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12.. math:: G(\delta) = 2 \pi \int_0^{\infty} J_0(Q \delta) \frac{d \Sigma}{d \Omega} (Q) Q dQ \!,
13
14in which :math:`J_0` is the zeroth order Bessel function, :math:`\delta` the spin-echo length, :math:`Q` the wave vector transfer
15and :math:`\frac{d \Sigma}{d \Omega} (Q)` the scattering cross section in absolute units.
16This is a 1-dimensional integral, which can be rather fast.
17In the numerical calculation we integrate from :math:`Q_{min} = 0.1 \times 2 \pi / R_{max}` in which :math:`R_{max}` will be model dependent.
18We determined the factor 0.1 by varying its value until the value of the integral was stable.
19This happened at a value of 0.3.  The have a safety margin of a factor of three we have choosen the value 0.1.
20For the solid sphere we took 3 times the radius for :math:`R_{max}`.
21The real integration is performed to :math:`Q_{max}` which is an instrumental parameter that is read in from the measurement file.
22From the equation above we can calculate the polarisation that we measure in a SESANS experiment:
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24.. math:: P(\delta) = e^{t \left( \frac{ \lambda}{2 \pi} \right)^2 \left(G(\delta) - G(0) \right)} \!,
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[4a2e1e5]26in which :math:`t` is the thickness of the sample and :math:`\lambda` is the wavelength of the neutrons.
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