The Statistical Analysis of High Energy Electron Flux Variations in the Radiation Belts

Details The Statistical Analysis of High Energy Electron Flux Variations in the Radiation Belts The Statistical Analysis of High Energy Electron Flux Variations in the Radiation Belts

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsm33a0351k&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SM33A-0351

Physics

2730 Magnetosphere: Inner, 2774 Radiation Belts, 7514 Energetic Particles (2114), 7845 Particle Acceleration, 7954 Magnetic Storms (2788)

Scientific paper

When a magnetic storm occurs, the flux of high energy electrons (>2.5MeV) in the earth radiation belts shows a decrease in the outer belt in the main phase, an increase in the outer belt in the recovery phase, and an increase in the slot region in the main-recovery phases. In this research, we analyze flux variation in the slot region during storms observed by Radiation Monitor on the spacecraft EXOS-D (Akebono). By the multiple linear regression model, we find a linear relationship between occurrence of the flux increase in the slot region and maximum Kp. It is thought that Kp is effective for a physical process causing an increase in flux of the slot region.

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