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AGU: Journal of Geophysical Research, Space Physics

 

Keywords

  • particle precipitation
  • ground transmitters
  • radiation belts

Index Terms

  • Magnetospheric Physics: Energetic particles: precipitating
  • Magnetospheric Physics: Magnetosphere: inner
  • Space Plasma Physics: Wave/particle interactions
  • Ionosphere: Wave/particle interactions
  • Magnetospheric Physics: Radiation belts
Abstract
Cited By (0)
 

Abstract

DEMETER observations of transmitter-induced precipitation of inner radiation belt electrons

K. L. Graf

Space, Telecommunications and Radioscience Laboratory, Stanford University, Stanford, California, USA

U. S. Inan

Space, Telecommunications and Radioscience Laboratory, Stanford University, Stanford, California, USA

D. Piddyachiy

Space, Telecommunications and Radioscience Laboratory, Stanford University, Stanford, California, USA

P. Kulkarni

Space, Telecommunications and Radioscience Laboratory, Stanford University, Stanford, California, USA

M. Parrot

Laboratoire de Physique et Chimie de l'Environnement, Centre National de la Recherche Scientifique, Orléans, France

J. A. Sauvaud

Centre d'Etude Spatiale des Rayonnements, Centre National de la Recherche Scientifique, Toulouse, France

Near loss cone energetic electron flux increases induced by ground-based very low frequency (VLF) transmissions are observed directly via satellite-based detection. In 2 years of experiments ranging from 27 March 2006 through 2 April 2008 with the 21.4-kHz transmitter NPM in Lualualei, Hawaii, and the French satellite DEMETER (detection of electromagnetic emissions transmitted from earthquake regions), only a few cases of detection of individual pulses of transmitter-induced precipitation of inner radiation belt electrons have been realized. Analysis of the specific cases of detection allow comparison of precipitating flux with predictions based on ray-tracing analyses of wave propagation and test particle modeling of the wave-particle interaction. Results indicate that the precipitated flux of >100 keV electrons induced by the NPM transmitter peaks at L ≃ 1.9 and, in the rare cases of detection, may be at higher energies than the ∼100 keV peak predicted by the model. The low detection rate is attributed to the orientation of the DEMETER particle detector, which is mostly overwhelmed by the trapped population at the location of detection.

Received 25 November 2008; accepted 3 April 2009; published 3 July 2009.

Citation: Graf, K. L., U. S. Inan, D. Piddyachiy, P. Kulkarni, M. Parrot, and J. A. Sauvaud (2009), DEMETER observations of transmitter-induced precipitation of inner radiation belt electrons, J. Geophys. Res., 114, A07205, doi:10.1029/2008JA013949.

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