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| Detailed Reference Information |
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Datta, S., Skoug, R.M., McCarthy, M.P. and Parks, G.K. (1996). Analysis and modeling of microburst precipitation. Geophysical Research Letters 23: doi: 10.1029/96GL01672. issn: 0094-8276. |
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Observations from a recent rocket experiment that measured electrons over the energy range of 1--300 keV shows that microburst temporal structures exist from about 20 keV to >120 keV. Simultaneous observations at five different pitch-angles (0¿--90¿) show the distribution is nearly isotropic during the bursts, while at low activity (quiet times and the valleys between microbursts) the distribution is anisotropic with higher fluxes at larger pitch-angles. The energy spectra were reasonably fit with a Maxwellian, with an e-folding energy E0≈6--9 keV for &agr;=0¿, which increases to ≈10 keV at 67¿. A modeling of electron spectra using the theory of pitch-angle diffusion can reproduce the observed spectra, suggesting pitch-angle scattering of electrons due to a wave-particle interaction is the primary mechanism responsible for microbursts. ¿ American Geophysical Union 1996 |
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Abstract |
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Keywords
Magnetospheric Physics, Auroral phenomena, Magnetospheric Physics, Energetic particles, precipitating, Ionosphere, Wave/particle interactions |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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