[ Identification | Description | Input parameters | Links ]
ISIS_TOSCA_preupgrade_Mantid InstrumentThe model at hand is adapted from an earlier model by M.Zanetti and represents the TOSCA instrument as it looked prior to the recent upgrade. The model at hand was adapted during the MDANSE2018 workshop (http://mdanse2018.essworkshop.org) and by default uses a model of the incoherent scattering from Benzene, created using CASTEP (http://www.castep.org ) and converted to Sqw format iFit (http://ifit.mcode.org) The model is naturally very challenging to run because of the indirect TOF geometry and would benefit from an adaptive sampling approach. Please follow instructions at https://github.com/McStasMcXtrace/McCode/wiki/McStas-and-Mantid to compile with NeXus and generate a Mantid-IDF before attempting to use with Mantid. To generate the right flightpath length in Mantid, this version of the instrument has been created with transmitting rather than reflecting analysers, and the detectors are hence also positioned differently than in the physical instrument. Example: ISIS_TOSCA_preupgrade_Mantid.instr inc=Benzene_inc_CASTEP_MDANSE2018.sqw eventmode=1 Detector: Sphere_I=0.686792 Example: ISIS_TOSCA_preupgrade_Mantid.instr inc=Benzene_inc_CASTEP_MDANSE2018.sqw eventmode=1 --format=NeXus Detector: Sphere_I=0.686792
| Name | Unit | Description | Default |
| inc | filename | Incoherent scattering model to use | "Benzene_inc_CASTEP_MDANSE2018.sqw" |
| zdepth | m | Thickness of sample | 0.002 |
| Emin | meV | Minimum energy to generate at the source | 0.01 |
| Emax | meV | Maximum energy to generate at the source | 500 |
| eventmode | boolean | Flag to enable event monitors | 0 |
ISIS_TOSCA_preupgrade_Mantid.instr.
[ Identification | Description | Input parameters | Links ]
Generated on 2023-09-19 20:01:36