Abstract
A rapid loss of energetic (>230 keV) electrons from the outer radiation belt was observed with the GPS constellation between 1430 and 1730 UTC on 7 May 2007. The rapid loss occurred from 4 < L* < 6 over all measured energies above 230 keV. Currently accepted rapid loss mechanisms include magnetopause shadowing and/or outward diffusion, and precipitation to the atmosphere due to wave-particle interactions. Here the loss timescale is ∼2 hr, and the magnetopause is near L = 8, which requires unrealistically high outward diffusion rates. Current estimates of the loss timescales associated with EMIC waves, plasmaspheric hiss and whistler-mode chorus are too long, even in combination, to explain the observed losses inside L* $\simeq$ 6. Copyright © 2010 by the American Geophysical Union.
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CITATION STYLE
Morley, S. K., Friedel, R. H. W., Cayton, T. E., & Noveroske, E. (2010). A rapid, global and prolonged electron radiation belt dropout observed with the Global Positioning System constellation. Geophysical Research Letters, 37(6). https://doi.org/10.1029/2010GL042772
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