Observations of a low-frequency cutoff in magnetospheric radio noise received on Imp 6

Details Observations of a low-frequency cutoff in magnetospheric radio noise received on Imp 6 Observations of a low-frequency cutoff in magnetospheric radio noise received on Imp 6

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.2771v&link_type=abstract

Journal of Geophysical Research, vol. 80, July 1, 1975, p. 2771-2774. Research supported by the University of Leicester;

Astronomy and Astrophysics

Astronomy

1

Atmospherics, Earth Magnetosphere, Electromagnetic Noise Measurement, Low Frequencies, Satellite Observation, Explorer Satellites, Magnetosheath, Plasma Waves, Radio Astronomy, Radio Scattering, Ray Tracing

Scientific paper

The quasi-continuous component of the magnetospheric noise observed by Imp 6, lying between 30 and 110 kHz, often exhibits a low-frequency cutoff when the spacecraft is in the interplanetary medium or the magnetosheath. A hypothesis is considered in which this low-frequency cutoff, f-co, is caused by overdense plasma situated somewhere along the noise-source-to-satellite path. The plasma is assumed to have a plasma frequency approximately equal to f-co, thus cutting off propagation below f-co.

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