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authorThomas White <taw@physics.org>2018-12-18 14:54:10 +0100
committerThomas White <taw@physics.org>2018-12-18 15:38:13 +0100
commit33d20aa3ea505e214fdcfc2c532b6bda28df7979 (patch)
treeaf56a54c0662fa509a297ff431a4be9ea807a0c4 /doc
parent42a3b30b26b2fae7c11568991581eafe935c4cea (diff)
Update partialator manual
Diffstat (limited to 'doc')
-rw-r--r--doc/man/partialator.17
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.