Radio noise of auroral origin - 1968-1988

Details Radio noise of auroral origin - 1968-1988 Radio noise of auroral origin - 1968-1988

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jatp...51..197l&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 51, March 1989, p. 197-203, 205-211.

Computer Science

Sound

13

Atmospheric Sounding, Atmospherics, Auroral Echoes, Histories, Auroral Arcs, Auroral Electrojets, Radio Frequencies, Riometers

Scientific paper

Observations of radio waves in the frequency range 0.1-200 MHz are reviewed, with emphasis on observations between 1968 and 1988. It is suggested that many of the observations, such as the bursts of enhanced noise associated with absorption events reported by Nishimuta et al. (1969), Harang (1969), and Osipov and Shevelev (1973), may represent the same phenomenon. Theoretical explanations for the occurrence of auroral radio noise include synchrotron radiation, Cerenkov radiation, plasma oscillations, and cyclotron maser generation.

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