Spatial distribution of geomagnetic-field oscillations connected with solar flares

Details Spatial distribution of geomagnetic-field oscillations connected with solar flares Spatial distribution of geomagnetic-field oscillations connected with solar flares

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..977g&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Nov.-Dec. 1987, p. 977-981. In Russian.

Physics

Geomagnetism, Ionospheric Disturbances, Plasma Oscillations, Solar Flares, Solar Terrestrial Interactions, Spatial Distribution, Ionizing Radiation, Ionospheric Currents

Scientific paper

It is shown that the ionizing radiation from solar flares leads to pulsed heating of the ionosphere primarily at high latitudes as the result of Joule-heat release from flare-disturbed Sq-currents. The flare radiation is a catalyst for the relase of energy stored in the ionospheric currents. Observed geomagnetic-field oscillations arise due to the interaction of acoustic oscillations of the disturbed ionosphere with the geomagnetic field.

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