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UPOS Space Weather Products

Radiation Belt Environment
RBE

Purpose:
Sample RBE Image: 
  20030505_1930_e_0918keV_PA
The energetic plasmas in radiation belt have deleterious impact on satellite systems and humans in space. It is critical to predict and forecast the developments of these energetic particles and provide warnings early enough for appropriate actions to be taken. Fok, Khazanov, and co workers' radiation belt and ring current model is a data-driven physics-based model which solves the convection-diffusion equation of plasma distribution functions in the range of 2-10 Earth radii. The only inputs to the model are solar wind and interplanetary magnetic field (IMF) conditions. The model calculates energetic plasma fluxes (10 keV to 5 MeV for electrons, 10 keV to 1 MeV for H+) and the correspoinding radiation doses. The current version of the model provides now-casting of the radiation-belt environment. Our ultimate goal is to do predicitons 24 hours ahead of time. On the right is an example of the RBE output. The left panel is the pitch-angle averaged flux at the magnetic equator. The white circle is the geosynchronous orbit. The right panel shows the pitch-angle distribution.

Input:
IMF, solar wind density, velocity, and predicted Dst.

Output:
The output of the Radiation Belt Environment model is an ASCII file containing electron or proton fluxes as a function of time, location, energy and pitch angle as well as plots of the plasma differential flux at the magnetic equator and the pitch-angle anisotropy(PAA). (See sample image above)
Documents: (Adobe Acrobat PDF)
Requirements
User's Guide
Design Document
Test Plan
Support Plan
Version Description
Quick Start Guide
The Application:
Latest RBE Images (Updated every 15 minutes)
Input File

For science comments/questions, contact M. Fok, GSFC
or G. Khazanov, MSFC

For software comments/questions, contact L. Burke, JHU/APL


http://sd-www.jhuapl.edu/UPOS/RBE/ © 2000 JHUAPL All rights reserved.