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| author | Thomas White <taw@physics.org> | 2018-12-18 14:54:10 +0100 |
|---|---|---|
| committer | Thomas White <taw@physics.org> | 2018-12-18 15:38:13 +0100 |
| commit | 33d20aa3ea505e214fdcfc2c532b6bda28df7979 (patch) | |
| tree | af56a54c0662fa509a297ff431a4be9ea807a0c4 /doc | |
| parent | 42a3b30b26b2fae7c11568991581eafe935c4cea (diff) | |
Update partialator manual
Diffstat (limited to 'doc')
| -rw-r--r-- | doc/man/partialator.1 | 7 |
1 files changed, 1 insertions, 6 deletions
diff --git a/doc/man/partialator.1 b/doc/man/partialator.1 index 7a4b3310..1a6d30d3 100644 --- a/doc/man/partialator.1 +++ b/doc/man/partialator.1 @@ -178,12 +178,7 @@ The available partiality models are: .IP \fBxsphere\fR .PD -The volume of intersection between a sphere centered on each reciprocal lattice -point and the part of reciprocal space excited by the Ewald sphere taking into -account the finite bandwidth and convergence angle. A "source coverage factor" -is included to take into account the spectral brightness of the effective -source for the reflection. The X-ray spectrum is modelled as a super-Gaussian -with exponent 1.5, and the overlap integral is evaluated numerically. +The volume of intersection between a sphere centered on each reciprocal lattice point and the part of reciprocal space excited by the Ewald sphere taking into account the finite bandwidth of the incident X-rays. A "source coverage factor" is included to take into account the spectral brightness of the effective source for the reflection. The X-ray spectrum is modelled as a super-Gaussian with exponent 1.5, and the overlap integral is evaluated numerically. This model is the same as that described in Acta Cryst. D71 (2015) p1400. |