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[ Identification | Description | Input parameters | Links ]
The SOLEIL_MARS Instrument
The MARS beam-line at Synchrotron SOLEIL.
Identification
- Site: SOLEIL
- Author: IGUILIZ Salah-Eddine, MENUT Denis and FARHI Emmanuel.
- Origin: SOLEIL
- Date: July 2022
Description
MARS beamline is aiming to extend the research capabilities on radioactive matter towards the use of synchrotron radiation in multidisciplinary fields biology, chemistry, physics) with respect to national and European safety law*. The design of MARS beamline (infrastructure and optics) is also optimized to alternatively run two experimental stations in order to perform characterizations with transmission and high resolution X-ray powder-diffraction (XRD), Wide Angle X-ray Scattering (WAXS), Small Angle X-ray scattering (SAXS), standard and high resolution X-ray absorption spectroscopy (XANES, EXAFS and HERFD-XANES) and microbeam techniques (microXRF, XAS, XRD). This model implements the XRD station for powders.
Input parameters
Parameters in boldface are required; the others are optional.| Name | Unit | Description | Default |
| E0 | keV | Central energy to be emitted by the source | 16.99 |
| reflec_material_M12 | str | reflecting coating on curved mirrors, e.g. Pt | "Pt.dat" |
| reflections | str | List of powder reflections, obtained with e.g. cif2hkl | "LaB6_660b_AVID2.hkl" |
| dEr | keV | Relative half width to emitted by the source, e.g. 1e-4 | 1e-4 |
| alpha | deg | Asymmetry angle for the crystals. | 0 |
Links
- Source code for
SOLEIL_MARS.instr.
[ Identification | Description | Input parameters | Links ]
Generated on 2023-12-19 19:37:45
