EarthRef.org Reference Database (ERR)
Development and Maintenance by the EarthRef.org Database Team

Detailed Reference Information
Datta et al. 1996
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.

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

BACKGROUND DATA FILES

Abstract

Keywords
Magnetospheric Physics, Auroral phenomena, Magnetospheric Physics, Energetic particles, precipitating, Ionosphere, Wave/particle interactions
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
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
Click to clear formClick to return to previous pageClick to submit