The magnetic field of the solar wind and vertical motion of the nighttime ionosphere

Details The magnetic field of the solar wind and vertical motion of the nighttime ionosphere The magnetic field of the solar wind and vertical motion of the nighttime ionosphere

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ge%26ae..15..977l&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 15, Nov.-Dec. 1975, p. 977-981. In Russian.

Computer Science

3

F Region, Ionospheric Drift, Magnetic Variations, Nocturnal Variations, Solar Wind, Geomagnetism, Plasma Dynamics, Vertical Distribution

Scientific paper

Changes in the characteristic altitude of the F layer of the nighttime ionosphere in the presence of abrupt changes of the vertical component of the magnetic field of the solar wind are investigated. The altitude of the nighttime ionosphere is shown to change systematically with changes in the vertical component. Positive fluctuations (from south to north) lead to an increase in the altitude of the F layer, while negative fluctuations induce an opposite altitude change of about the same magnitude.

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