Simulating the beamline 11-2 of SSRL to reproduce their glitches database.
The source is chosen to not be white in this instrument to increase the detected photons, another .instr has a white source.
Identification
Site: SOLEIL
Author:
Origin: Synchrotron Soleil
Date: Dec 5th 2022
Description
BL 11-2 beamline description here: https://www-ssrl.slac.stanford.edu/mes/11-2/manual.php
https://www-ssrl.slac.stanford.edu/mes/Glitch_Curves/ , the instrument is the BL in the unfocussed and uncollimated mode
SSRL glitch database found here: https://www-ssrl.slac.stanford.edu/smbin/dataextractnew.pl
Documentation and results of the .instr here: https://gitlab.synchrotron-soleil.fr/grades/beamlines/-/tree/main/glitches
A jupyter notebook will soon be available regrouping everything.
You may scan like so for example:
mxrun -n 1e7 bl_11_2_not_white_src.instr -N601 Etohit=6900,7500
Input parameters
Parameters in boldface are required;
the others are optional.
Name
Unit
Description
Default
Etohit
eV.
Energy used to calculate the bragg angle the monochromator is put at. This is the energy we select.