Physics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jgr....87.2347g&link_type=abstract
Journal of Geophysical Research, vol. 87, Apr. 1, 1982, p. 2347-2355. Research supported by the Universite de Paris VI; Centre N
Physics
3
Extremely Low Frequencies, Plasma Interaction Experiment, Satellite Observation, Signal Detection, Tropical Regions, Bandwidth, Earth Magnetosphere, Harmonic Radiation, Plasma-Particle Interactions, Signal Transmission
Scientific paper
The SCATHA and GEOS 2 spacecraft VLF receivers have detected emissions related to high-latitude ELF transmissions despite the low transmitted power, and found emission behavior similar to that observed by ground receivers in the case of power line harmonic radiation. Because the keying of the transmitted waves was not generally detected, and the bandwidths of the detected signals were significantly wider than that of the transmitted signals, identification of the signals as plasma wave emissions rather than as linear amplifications of the transmitted signal is possible with certainty. Since a large number of interactions may be required before the emission signal is amplified to a detectable level, the general absence of keying on the received signal may be explained by the increased time required for this process to occur in the outer magnetosphere.
Dazey M. H.
Garnier M.
Girolami G.
Koons Harry C.
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