Physics
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.2183p&link_type=abstract
Journal of Geophysical Research, vol. 80, June 1, 1975, p. 2183-2198.
Physics
4
Earth Magnetosphere, Hiss, Magnetic Measurement, Satellite Observation, Daytime, Electromagnetic Noise Measurement, Explorer Satellites, Extremely Low Frequencies, Magnetic Storms, Satellite-Borne Instruments
Scientific paper
Data obtained with an Explorer-45 instrument for detecting the magnetic components of ELF signals propagating in the magnetosphere are examined, showing that the strongest, most persistent signals were plasmaspheric hiss from a few hundred to a few thousand Hertz. Broad-band signals of 25 milligamma were common. The most intense hiss was observed in the recovery phase of magnetic storms at the inner edge of the ring current. Its source appears to be the outer plasmasphere. Most of the hiss is attributed to generation of hiss through cyclotron resonance with energetic electrons. Ring current protons, forming a peak in the proton flux between 10 and 100 keV, may be a source of some of the hiss.
Cahill Laurence J. Jr.
Eberlein D. D.
Marvin James A.
Parady B. K.
Taylor William W. L.
No associations
LandOfFree
Plasmaspheric hiss observations in the evening and afternoon quadrants does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Plasmaspheric hiss observations in the evening and afternoon quadrants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Plasmaspheric hiss observations in the evening and afternoon quadrants will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-750516