Physics
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsm11a0800r&link_type=abstract
American Geophysical Union, Fall Meeting 2001, abstract #SM11A-0800
Physics
2704 Auroral Phenomena (2407), 2716 Energetic Particles, Precipitating, 7867 Wave/Particle Interactions
Scientific paper
Pitch angle diffusion by plasma waves is often cited as the cause of the diffuse auroral electron precipitation. The diffuse electron aurora is a steady drizzle into the atmosphere at all local times and geomagnetic conditions. Comparisons of electron distributions which were simultaneously measured by low and high altitude satellites in the same flux tube often exhibit a completely filled loss cone. This result implies that the pitch angle diffusion rate was near the strong diffusion limit. Some statistical studies of the plasma wave power in the magnetosphere show, however, that the observed waves are rarely strong enough to support strong diffusion of the particles. We use simultaneous wave and particle data from the SCATHA satellite to show in detail the effects of the waves on the electrons. Several cases are analyzed to correlate the level of the electron distribution function in the atmospheric loss cone with the magnitude of the wave power. The angular extent of the atmospheric loss cone at the SCATHA position is comparable to the detector field of view. To achieve a more precise estimate of the level of electrons in the loss cone, an angular deconvolution analysis is performed on the electron distributions using several methods. The pitch angle diffusion effects of several different types of waves are investigated, including electrostatic electron cyclotron harmonic waves and electromagnetic whistler-mode chorus. These results are then compared with the diffusion rates calculated by quasilinear plasma theory.
Fennell Joseph F.
Koons Harry C.
Roeder James L.
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