Ionospheric Electron Concentration Enhancement during a Solar Flare

Details Ionospheric Electron Concentration Enhancement during a Solar Flare Ionospheric Electron Concentration Enhancement during a Solar Flare

Nov 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.228..653t&link_type=abstract

Nature, Volume 228, Issue 5272, pp. 653-654 (1970).

Computer Science

2

Scientific paper

DURING solar flares, sudden increases of extreme ultraviolet (EUV) and X-ray flux produce abrupt increases of electron concentration (Ne) in the sunlit part of the ionosphere. Because of their relatively short duration and the accompanying blackout in h.f. propagation, these enhancements of Ne have hitherto been difficult to investigate, especially in the E region. We report here some results of applying a new technique, incoherent scatter radar, to this problem. The observations were made at Malvern (52.1° N, 2.3° W) during a solar flare on February 20, 1970.

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