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EPREM (20181001)

Energetic Particle Radiation Environment Module

Model Description

At 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 Description


	
	
	
	

Model Outputs Description


	
	
	
	

Model Caveats


	
	
	
	

Change Log


	
	 
	

Model Acknowledgement/Publication Policy (if any)


	
	
	

Model Domains:

Heliosphere.Inner_Heliosphere

Space Weather Impacts:

Solar energetic particles - SEPs (human exploration, aviation safety, aerospace assets functionality)

Phenomena :

Solar_Energetic_Particles

Simulation Type(s):

Physics-based

Temporal Dependence Possible? (whether the code results depend on physical time?)

true

Model is available at?

CCMC

Source code of the model is publicly available?

false

CCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):

retired

Code Language:

C

Regions (this is automatically mapped based on model domain):

Heliosphere.Inner

Contacts :

Matt.Gorby, ModelDeveloper
Nathan.Schwadron, ModelDeveloper

Acknowledgement/Institution :

Relevant Links :

Publications :

Model Access Information :

Linked to Other Spase Resource(s) (example: another SimulationModel) :

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Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement