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EPREM (20181001)Energetic Particle Radiation Environment ModuleModel DescriptionAt CCMC EPREM can be run in three ways: 1) EPREM: assuming a Parker Spiral IMF, background conditions. 2) EPREM+Cone: assuming a Parker Spiral IMF, with an inserted idealized "cone" CME into the EPREM domain. 3) EPREM+ENLIL: uses a WSA-ENLIL+Cone run as it's domain. For this option, first an WSA-ENLIL+Cone simulation with appropriate settings must be selected from the run database. Model Figure(s) :Model Inputs DescriptionModel Outputs DescriptionModel CaveatsChange LogModel Acknowledgement/Publication Policy (if any)Model Domains:Heliosphere.Inner_HeliosphereSpace Weather Impacts:Solar energetic particles - SEPs (human exploration, aviation safety, aerospace assets functionality)Phenomena :Solar_Energetic_ParticlesSimulation Type(s):Physics-basedTemporal Dependence Possible? (whether the code results depend on physical time?)trueModel is available at?CCMCSource code of the model is publicly available?falseCCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):retiredCode Language:CRegions (this is automatically mapped based on model domain):Heliosphere.InnerContacts :Matt.Gorby, ModelDeveloperNathan.Schwadron, ModelDeveloper Acknowledgement/Institution :Relevant Links :Publications :Model Access Information :Linked to Other Spase Resource(s) (example: another SimulationModel) : |
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