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Read Full Article (file size: 506044 bytes) Cited by
GEOPHYSICAL RESEARCH LETTERS,
VOL. 35,
L19103,
doi:10.1029/2008GL034834,
2008
Effects of plasma density irregularities on the pitch angle scattering of radiation belt electrons by signals from ground
based VLF transmitters
T. F. Bell
STAR Laboratory, Stanford University, Stanford, California, USA
U. S. Inan
STAR Laboratory, Stanford University, Stanford, California, USA
D. Piddyachiy
STAR Laboratory, Stanford University, Stanford, California, USA
P. Kulkarni
STAR Laboratory, Stanford University, Stanford, California, USA
M. Parrot
LPCE, CNRS, Orleans, France
Abstract
Recent DEMETER spacecraft observations show that VLF signals from the NPM transmitter in Hawaii often strongly excite quasi-electrostatic
whistler mode waves as the NPM signals propagate upward through plasma density irregularities. As a result of the NPM wave
energy loss to the quasi-electrostatic waves, the transmitter signals will arrive at the radiation belts with less intensity
than predicted by present models of VLF wave propagation and will produce less pitch angle scattering of energetic electrons
than presently believed. This type of wave energy loss may be partially responsible for the pervasive wave intensity deficit
for VLF transmitter signals in the plasmasphere recently noted by Starks et al. (2008).
Received 16
June
2008;
accepted 25
August
2008;
published 4
October
2008.
Keywords: wave scattering.
Index Terms: 0654 Electromagnetics: Plasmas; 0669 Electromagnetics: Scattering and diffraction; 0689 Electromagnetics: Wave propagation (2487, 3285, 4275, 4455, 6934); 2716 Magnetospheric Physics: Energetic particles: precipitating; 2768 Magnetospheric Physics: Plasmasphere.
Read Full Article (file size: 506044 bytes) Cited by
Citation: Bell, T. F., U. S. Inan, D. Piddyachiy, P. Kulkarni, and M. Parrot
(2008),
Effects of plasma density irregularities on the pitch angle scattering of radiation belt electrons by signals from ground
based VLF transmitters,
Geophys. Res. Lett.,
35,
L19103,
doi:10.1029/2008GL034834.
Copyright 2008 by the American Geophysical Union.
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