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[ Identification | Description | Input parameters | Links ]
The glitches_energy Instrument
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. | 6900 |
| h | Miller indices. | 2 | |
| k | Miller indices. | 2 | |
| l | Miller indices. | 0 |
Links
- Source code for
bl_11_2_not_white_src.instr.
[ Identification | Description | Input parameters | Links ]
Generated on 2023-12-19 19:37:45
