On the cause of the incoherent scatter plasma line in the presence of auroral electron precipitation

Details On the cause of the incoherent scatter plasma line in the presence of auroral electron precipitation On the cause of the incoherent scatter plasma line in the presence of auroral electron precipitation

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jatp...48.1021h&link_type=abstract

(EISCAT Scientific Association, International EISCAT Workshop, 2nd, Aberystwyth, Wales, Sept. 9-12, 1985) Journal of Atmospheric

Physics

Auroral Zones, Electron Precipitation, F Region, Incoherent Scatter Radar, Plasma Spectra, Ionospheric Electron Density, Wave Propagation

Scientific paper

Field-aligned auroral electrons precipitating into the atmosphere are likely to amplify the ionospheric thermal density fluctuations significantly at F-layer heights for the k value observable with the EISCAT VHF radar, but not for the larger k value of the UHF radar. A strong amplification of the wave amplitude may happen in a small fraction of a second, while the wave propagates only one or a few kilometers.

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