MHD structure of interplanetary streams from flares of August 1972. I - Shock waves and 'magnetic' regions

Details MHD structure of interplanetary streams from flares of August 1972. I - Shock waves and 'magnetic' regions MHD structure of interplanetary streams from flares of August 1972. I - Shock waves and 'magnetic' regions

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ge%26ae..19..981e&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 19, Nov.-Dec. 1979, p. 981-987. In Russian.

Physics

Interplanetary Magnetic Fields, Magnetohydrodynamic Flow, Satellite Observation, Solar Flares, Solar Magnetic Field, Solar Wind Velocity, Pioneer 10 Space Probe, Pioneer 9 Space Probe, Shock Fronts, Shock Wave Propagation

Scientific paper

The paper examines data on the MHD structure of interplanetary streams arising from the intense solar flares of August 2 and 4, 1972. Characteristics of interplanetary shock waves and flow structure, as measured by Pioneer 9 and 10 and Prognoz 1 and 2, are investigated. Data indicate the existence of magnetic regions in the interplanetary streams characterized by sharp shock fronts, large-scale and quiet magnetic field, and low plasma concentration.

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