Physics – Plasma Physics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007georl..3420112l&link_type=abstract
Geophysical Research Letters, Volume 34, Issue 20, CiteID L20112
Physics
Plasma Physics
13
Magnetospheric Physics: Radiation Belts, Space Plasma Physics: Wave/Particle Interactions (2483, 6984), Magnetospheric Physics: Energetic Particles: Trapped, Magnetospheric Physics: Energetic Particles: Precipitating, Magnetospheric Physics: Magnetic Storms And Substorms (7954)
Scientific paper
We simulate the behaviour of relativistic (976 keV) electrons in the outer radiation belt (3 <= L <= 7) during the first half of the CRRES mission. We use a 1d radial diffusion model with losses due to pitch-angle scattering by plasmaspheric hiss expressed through the electron lifetime calculated using the PADIE code driven by a global K p -dependent model of plasmaspheric hiss intensity and f pe /f ce . We use a time and energy-dependent outer boundary derived from observations. The model reproduces flux variations to within an order of magnitude for L <= 4 suggesting hiss is the dominant cause of electron losses in the plasmasphere near the equator. At L = 5 the model reproduces significant variations but underestimates the size of the variability. We find that during magnetic storms hiss can cause significant losses for L <= 6 due to its presence in plumes. Wave acceleration is partially represented by the boundary conditions.
Glauert Sarah A.
Horne Richard B.
Lam Matthew
Meredith Nigel P.
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