Hydromagnetic structure of the interplanetary flux from the powerful flare of August 4, 1972

Details Hydromagnetic structure of the interplanetary flux from the powerful flare of August 4, 1972 Hydromagnetic structure of the interplanetary flux from the powerful flare of August 4, 1972

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ge%26ae..16..970e&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 16, Nov.-Dec. 1976, p. 970-975. In Russian.

Physics

Interplanetary Space, Magnetic Measurement, Plasma Density, Plasma Flux Measurement, Satellite-Borne Instruments, Solar Flares, Magnetohydrodynamic Flow, Magnetometers, Shock Fronts, Solar Wind

Scientific paper

An analysis of magnetic measurements carried out in near interplanetary space showed that the interplanetary flux from the August 1972 flare constituted a modification of the typical flux; the phenomena observed in interplanetary space were apparently caused by extremely oblique passage of the flux. The slope of the structural regions with respect to the sun-earth line and the ecliptic plane was large enough to produce a double intersection of the flare-plasma front.

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