Evolution of energetic electron pitch angle distributions during storm time electron acceleration to megaelectronvolt energies
Horne, R.B.; Meredith, N.P.; Thorne, R.M.; Heynderickx, D.; Iles, R.H.A.; Anderson, R.R.. 2003 Evolution of energetic electron pitch angle distributions during storm time electron acceleration to megaelectronvolt energies. Journal of Geophysical Research, 108 (A1), 1016. 13, pp. 10.1029/2001JA009165Full text not available from this repository. (Request a copy)
We investigate the pitch angle distributions of 0.15-1.58 MeV electrons observed during the 9-15 October 1990 storm measured by the Combined Release and Radiation Effects Satellite (CRRES) spacecraft. This storm period is characterized by an enhancement in the electron flux at L approximate to 4 by more than an order of magnitude over the prestorm level. The overall change in flux at L approximate to 6.6 is small in comparison. Previous work shows that radial diffusion underestimates the flux enhancement by up to a factor of 5 for L less than or equal to 4.5 [Brautigam and Albert, 2000], indicating the need for an additional acceleration process. The pitch angle distributions presented here are examined for evidence of the acceleration mechanism. The distributions at L approximate to 2 are rounded and are dominated by Coulomb collisions. They show little variation during the storm. The distributions at L approximate to 3 are pancake-shaped before the storm, characteristic of pitch angle scattering by plasmaspheric hiss. During the main phase, they become broad and flat, and they evolve back into pancake distributions during the recovery phase. At L approximate to 4-6, the pitch angle distributions are characterized as butterfly distributions at storm onset, and they become broad flat top distributions during the recovery phase. The flat top distributions persist throughout the similar to3-day recovery phase and are observed in the region of highest flux enhancement. The flat top distributions are energy dependent and are broader at lower energies (30degrees-150degrees) than at higher energies (50degrees-130degrees). The higher energies exhibit a much faster fall off toward the loss cone than at lower energies. Inward radial diffusion should result in anisotropic distributions peaked near 90degrees and does not explain the observed energy dependence. Furthermore, the direction of diffusion is outward at higher energies. Model calculations of the pitch angles resonant with whistler mode waves show that flat top distributions are consistent with pitch angle and energy scattering in regions where f(pe)/f(ce)similar to1. Although radial diffusion may be very important for particle energization, the observed pitch angle distributions provide strong evidence that wave particle interactions play an important role in the energization process.
|Programmes:||BAS Programmes > Antarctic Science in the Global Context (2000-2005) > Magnetic Reconnection, Substorms and their Consequences|
|NORA Subject Terms:||Meteorology and Climatology
|Date made live:||11 Aug 2010 12:20|
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