Other
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40.1325h&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 10, p. 1325-1338.
Other
55
Earth Magnetosphere, Hiss, Midlatitude Atmosphere, Plasmasphere, Electromagnetic Radiation, Electron Cyclotron Heating, Morphology, Random Noise
Scientific paper
A review of mid-latitude and plasmaspheric hiss-type emissions observed on ground-based stations and in the earth's magnetosphere is presented. Different approaches to modeling of these emissions are discussed. It is pointed out that mid-latitude hiss emissions are most likely to be generated in the equatorial magnetosphere where the energy of electrons is transferred to wave energy via the electron cyclotron instability. Some quantitative characteristics of these emissions are explained in terms of a quasilinear model of this instability. Many properties of plasmaspheric hiss emissions are likely to be related to the same electron cyclotron instability, although the contribution of other mechanisms cannot be excluded.
Hayakawa Masahiko
Sazhin Sergei S.
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