The latitude dependence of vlf radiation intensity

Details The latitude dependence of vlf radiation intensity The latitude dependence of vlf radiation intensity

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..339s&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, Mar.-Apr. 1980, p. 339-341. In Russian.

Other

Atmospheric Radiation, Earth Magnetosphere, Intercosmos Satellites, Radiant Flux Density, Very Low Frequencies, Hiss, Latitude, Spectral Energy Distribution

Scientific paper

Consideration is given to the differential latitude dependence of the spectral energy density of magnetospheric elf and vlf radiation. Expressions for the spectral wave energy density distributions predicted by the model of plasmaspheric elf hiss excitation in the equatorial magnetosphere proposed by Etcheto (1972, 1973), its modification by Sazhin to take into account magnetic field inhomogeneity and the model of ionospheric wave generation of Kovner et al. (1978) and St. Maurice (1978) are presented. The latitude distribution of the spectral energy density of low-frequency waves observed by Intercosmos 5 is shown to agree most nearly with the distribution obtained from the model of Sazhin, despite its close agreement with that of Etcheto in most other aspects.

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