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Fok Radiation Belt Electron (1.0)

Fok Radiation Belt Electron (RBE)

Model Description

The Fok Radiation Belt Model (RBE) is a bounce-averaged kinetic model of the radiation belt electrons. This model calculates the temporal and spatial variation of the phase space density of radiation belt electrons(e-), in the energy range of 10 - 4000 keV.
The model considers particle drift, charge exchange loss, in realistic, time-varying magnetic and electric fields. The simulation region is from the dayside magnetopause to the nightside boundary at 10 earth radii. 
The model is an initial-boundary-value problem, so initial distribution and boundary distribution as a function of time is required to run the model.

Model Figure(s) :

Model Inputs Description

3D Magnetic Fields (from SWMF GM/BATSRUS model)
2D Ionospheric height-integrated Potentials (SWMF IE/Ridley model)
Equatorial Plasma Density (SWMF GM/BATSRUS)
Equatorial Plasma Temperature (SWMF GM/BATSRUS)

Model Outputs Description

Equatorial e- fluxes as functions of time, energy and pitch angle. Fluxes at off-equator can be obtained by assuming constant flux along a field line.

Model Caveats

Change Log

Model Acknowledgement/Publication Policy (if any)

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

Model is available at?

Source code of the model is publicly available?

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

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

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