OMERE Download
Full package – OMERE 5.3
Author: TRAD
Description: The whole package of OMERE 5.3
Last releases
 Release 14Jan2020 v5.3.2
 Release 16Sept2019 v5.3.1
 Release 10Apr2019 v5.2.5
 Release 20Dec2018v5.2.4
 Release 31Oct2018v5.2.3
 Release 17Sept2018v5.2.2
 Release 14Jun2018v5.0.6.0
 Release 16Apr2018v5.0.5.0
 Release 23March2018v5.0.4.0
 Release 21Mar2018v5.0.3.0
 Release 31Jul2017v5.0.1.4
 Release 18Apr2017v5.0.1.3
 Release 06Jun2016v4.2.2.0
 The userdefined orbit grid is now conserved when applying the Störmer geomagnetic cutoff.
 Multimission: calculation for transport has be corrected.
 Mission: the calculations fixed when considering nonisochron orbit.
• OMERE v5.3 is available in version 64bits.
• Integration of the average SAPPHIRE models for heavy ions.
• Integration of the solar flares SAPPHIRE models for protons and heavy ions.
• Integration of the GREENelectrons and GREENprotons models (trapped particles). Note that these models provide only integrated fluxes.
Improvements:
• The advanced manual has been merged with the regular user manual. It can now be accessed directly via the “advanced section” of the help menu.
• Management of versions has been improved where users installed several versions of OMERE on their computer.
Corrections:
• Solar particles: integration constant was missing after the application of the magnetospheric shielding.
• Fix of several minor issues.
 Solar cells: isotropy of spectrum was not correctly considered
 SEE module: restoration of the Bendel fit.
 Default Path files were not set correctly
 Dose curve calculation: when changing the target material several times, the calculation did not take the new material into account.
Improvements
 The METIS model is now available when HI crosssections data are in cm²/device.
 The SEE section in the help menu has been updated.
 In the “Equivalent LET” module: several plots can be overlaid.
Corrections
 Minor bugs have been fixed in the SEE module.
 Module Atomic Displacement: the calculation “along the orbit” is now available when “displacement dose file” is selected.
 The version of AE9/AP9 has been updated to v1.50
 The datac folder is now installed in another folder. This fixes a crash for computers on WINDOWS10.
Corrections
 Solar particles: software crashed when plotting solar ions
 Solar particles: the shielding was not taken into account for ions models.
 GCR: correction of the spectrum calculation with the “mission” option for GCR ISO 15390 model.
Major new modules
 AE9/AP9 v1.30 models (trapped particles)
 SAPPHIRE model for protons and Helium (solar particles)
 METIS model for proton cross sections calculation.
Major improvements
 Redesign of the Orbit dialog. For orbit files, possibility to change the order of the columns.
 Redesign and optimization of the SEE module.
 Redesign and optimization of the dose module.
 Improvement of the calculation time with SLOT and OZONE module.
 Shieldose: code optimisation & multithreading.
Others
Update of IGRF magnetic field at IGRF12 version
 Transport: transport of multiple proton files did not take into account the first incident flux file.
 LET spectrum: the calculation with the shielding geometry from a sector file was not possible.
 Windows 10: The trapped particle dialog was causing a crash.
 Transport: Shielding thickness <01 g.cm1 led to unchanged integral flux values.
 Trapped particle module: Magnetic field models given in result files could be different from the selected models on the GUI. However the computations used the models selected by the user.
 SEE rate calculation module: correction of the X axis unit of the Weibull curve display for heavy ions from energy to LET.
 GCR flux calculation module: The elements of the periodic table are now always updated automatically when switching from one element to another having a lower Z. This fix prevents a crash during the computations.
 SEE rate calculation module: correction of the SEE rate computations based on an integral LET file.
 Dose calculation module: dose depth curve graphs can now be overlaid only if their unit is the same.
 The date format in the output file of the instantaneous flux has been changed to increase their precision.
 Cosmic Rays module: correction on the calculation of the flux for the GCR ISO 15390 model with the Mission
Improvements

 Transport module: the results of the electron flux transport have now a fixed sampling (10 samples per decade) that is extended down to 1 keV.
 Graph plotting: plotting a graph from a file allows again overlaying graphs. Information about axis and units are also retrieved from the file if they exist and are correctly formatted.
 Trapped particle module: Magnetic field models given in result files could be different from the selected models on the GUI. However the computations used the models selected by the user.
 SEE rate calculation module: correction of the X axis unit of the Weibull curve display for heavy ions from energy to LET.
 GCR flux calculation module: The elements of the periodic table are now always updated automatically when switching from one element to another having a lower Z. This fix prevents a crash during the computations.
 SEE rate calculation module: correction of the SEE rate computations based on an integral LET file.
 Dose calculation module: dose depth curve graphs can now be overlaid only if their unit is the same.
 The date format in the output file of the instantaneous flux has been changed to increase their precision.
Improvements
 Transport module: the results of the electron flux transport have now a fixed sampling (10 samples per decade) that is extended down to 1 keV.
 Graph plotting: plotting a graph from a file allows again overlaying graphs. Information about axis and units are also retrieved from the file if they exist and are correctly formatted.
 Modification of the default name for the output file of the thickness table in dose calculation parameters.
 Modification of the output file name when postprocessing SEE using multimission tool.
 Temporary removal of ‘OScream’ in the ‘Solar Cells’ menu.
 Modification of the help of ‘Optimization and uncertainty estimation’ in SEE menu and addition of a popup message.
Corrections
 Correction of a bug in the consideration of flux units for SEE rate calculation with a proton integral flux file.
 Correction of a bug in the display of integral fluxes of solar flare particles previously plotting differential fluxes.
 Correction of the displayed unit for the dose depth curve depending on the chosen one in ‘SPECIALS’ parameters.
 Correction of the displayed unit for the displacement damage equivalent fluence curve depending on the chosen one in ‘Calculation parameters’.
 Correction of the calculation method for the solar active period considering missions over 2024.
 Correction of a bug in the consideration of crosssection test data in the SEE rate calculation wizard tool.
 Correction of a color scale bug when performing L meridian mapping using orbit projection.
 Correction of diverse minor bugs of the interface.
 OPAL ONERA trapped proton model for LEO (<800 km) orbits
 Peak flux calculations for SAA trapped protons
 Independent module for flux mapping
 Guided module for SEE rate calculation
 Possibility to include one or more (up to 4) layers in front of the sensitive zone for an equivalent LET calculation: SiO2, Al, Cu
 Mapping of the SAA with the possibility to plot inflight data
 Displacement Damage calculations giving the nonionizing dose in addition to an equivalent fluence
Major improvements
 Multithread option for trapped particle calculations (except for the models: OZONE & SLOT) and mapping
 Increase of the number of sensitive cells that can be defined in the SEE module
 Improvement of 2D, 3D displays, graph (color scales including the magnetic field mapping), dialog boxes and views by default
 Improvement of graph options
 Interface improvements and code optimization for modules: Mission, Trapped Particles, Solar Particles (average statistical and solar flares) and Cosmic Rays
 Solar cells, displacement and dose calculation: accuracy increase for mission duration definition in the input flux data file dialog box (from integer to double with 5 decimal precision)
Modifications
 Sector files: correction to manage sector files from the latest FASTRAD version
 SEE rate calculation module: modification of the flux selection for rate calculation when the option “from the current mission” is selected in the Environment dialog window
 Trapped protons: taken into account only for proton rate calculation
 Mean solar protons (ESP): taken into account only for proton rate calculation
 Inflare solar protons (proton models): taken into account only for proton rate calculation
 Inflare solar ions (Z=1 to 92): protons (Z=1) taken into account for proton rate calculation (except if user selects an inflare solar proton model) and ions (Z=1 to 92) taken into account for the LET calculation
 Cosmic ions (Z=1 to 92): protons (Z=1) taken into account for proton rate calculation and ions (Z=1 to 92) taken into account for the LET calculation
Corrections
 Mission file with multiple orbits: correction when loading a multiple orbit mission, the date for each orbit depends on the end date of the previous orbit
 Trapped particles module: temporary removal of the COMBI model for electrons, a problem with the flux calculation needs to be corrected
 SEE: correction of periodic flux file reading when file contains calculation steps with no fluxes
 Displacement module: calculation using NEMO database when data files are missing now returns an error
 ONERA Cutoff: correction of the attenuation coefficient calculation
 SEE: Heavy ions or protons are not considered for SEE calculation when their data are missing from the component database