Mode structure of damped quasi-periodic VLF emissions

Details Mode structure of damped quasi-periodic VLF emissions Mode structure of damped quasi-periodic VLF emissions

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..441g&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, May-June 1986, p. 441-446. In Russian.

Mathematics

Probability

Amplitude Distribution Analysis, Atmospheric Attenuation, Earth Magnetosphere, Propagation Modes, Very Low Frequencies, Whistlers, Fine Structure, Probability Density Functions, Radio Emission

Scientific paper

The fine structure of quasi-harmonic damped VLF emissions is analyzed on the basis of data obtained at the Magadan observatory in April 1980 and May 1984. It is shown that these emissions occur after intense weakly dispersed whistlers followed by a delay corresponding to the period of natural relaxation oscillations. The probability density functions of the amplitude and period distributions of the emissions have several peaks selected according to time and frequency. This fact of several peaks may be due to the mode structure of the VLF radiation, as it propagates in magnetospheric channels oriented along the magnetic field.

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