OMERE Download

• AE9/AP9 models have been updated. v1.57 is now available.
• New icons are available.

Corrections:

• The general stability of the software has been improved.
• Other minor bugs.

• LET equivalent tool has been corrected; Calculations with SiO2 or Cu layers, and multilayers calculations are now correct.
• Störmer cutoff model has been corrected.
• Interplanetary module has been corrected. Calculations with ions files, computed with Helium and SAPPHIRE models, are now available.
• Multithreading calculations with AE9/AP9 models have been fixed.
• The general stability of the software has been improved.
• Other minor bugs.

• The new ATOX module is now available. It allows users to compute the erosion of materials due to atomic oxygen at low altitudes.

Corrections:

• Multi Mission post-processing tool has been fixed. Output files were empty and are now filled with calculations asked by the user.
• OMERE takes into account the start date of a mission given by a .cen file.
• GREEN models: the launch date was not considered correctly when the mission was defined with an orbit file.
• SEE rate expert module: Bug in SEE rate due to the lack of LET file has been fixed. All SEE rate calculations, for both protons and ions are now correct, with or without a LET file in input.
• The general stability of the software has been improved.

Other minor bugs.

• Multi-mission has been fixed for displacement damage and solar cells degradation calculation.

• SEE: Correction on the results of the SEE rate calculation with the “from files” input.
• SEE: the “from files” and “from mission” are now independent.
• SEE: during a calculation “from files”, the protons where also considered for the ion calculation.
• The 2D display of the trajectory has been fixed.

• Mission: add of a new orbit file database. The user can add orbit files that will be stored and accessed easily.
• Redesign of the shielding definition tool. This tool is used in several modules: SEE, dose, atomic displacement, transport, LET spectrum, solar cells. It has been redesigned, and improved.
• Update of the GREEN models. The GREEN models are trapped electrons and protons models. The current version is now v4.

Corrections:

• SEE correction on the result file for contributions of solar particles. The in-flare and out-of-flare results were swapped.
• Atomic displacement: the results were wrong when using the “from files” input type.
• Environment (GCR): selecting the solar max option generated an empty output file.
• SEE: the calculation of the proton cross-section was not performed correctly with the Bendel model.
• The “Equivalent LET” tool was returning wrong values.
• Atomic displacement: the calculation of the NIEL using NEMO was not done properly.
• Other minor bugs.

• Solar cells: redesign of the tool
• Solar cells: addition of the NRL-SCREAM (O-SCREAM) model
• Solar cells: possibility to apply a factor R on the low energy protons
• Mission: possibility to define a mission from TLE (Two Lines Elements)
• Update of the ONERA/GREEN models

Improvements:

• The GREEN and AE9/AP9 models are now available in 64-bits.
• The 3D view is now automatically disabled if it cannot be supported by the user’s system.
• Improvement of progress bars for several calculations

Corrections:

• DDEF tool: correction of the conversion from one fluence to another.
• Trapped particles – proton peak flux. The durations were not saved in the output file.
• AE9/AP9 calculation has been fixed
• Correction of the modified Julian date (used for AE9/AP9 calculation)
• Equivalent LET: Fix on the deposited charge calculation
• Other minor corrections

• The user-defined orbit grid is now conserved when applying the Störmer geomagnetic cutoff.
• Multi-mission: calculation for transport has be corrected.
• Mission: the calculations fixed when considering non-isochron orbit.

• OMERE v5.3 is available in version 64-bits.
• Integration of the average SAPPHIRE models for heavy ions.
• Integration of the solar flares SAPPHIRE models for protons and heavy ions.
• Integration of the GREEN-electrons and GREEN-protons 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 cross-sections 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.

• 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.cm-1 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 post-processing SEE using multi-mission tool.
• Temporary removal of ‘O-Scream’ in the ‘Solar Cells’ menu.
• Modification of the help of ‘Optimization and uncertainty estimation’ in SEE menu and addition of a pop-up 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 cross-section 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.