Energetic properties of interplanetary plasma at the earth's orbit following the August 4, 1972 flare

Details Energetic properties of interplanetary plasma at the earth's orbit following the August 4, 1972 flare Energetic properties of interplanetary plasma at the earth's orbit following the August 4, 1972 flare

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51..217d&link_type=abstract

Solar Physics, vol. 51, Jan.-Feb. 1977, p. 217-229. Centre National d'Etudes Spatiales

Mathematics

Logic

2

Interplanetary Magnetic Fields, Plasma Dynamics, Solar Activity Effects, Solar Flares, Solar Wind, Meteorological Satellites, Pioneer 9 Space Probe, Plasma Density, Shock Wave Propagation

Scientific paper

Solar-wind and interplanetary-magnetic-field data were obtained by the Prognoz 1 and Prognoz 2 satellites during the period following the August 4, 1972, (06:21 UT) solar flare. A thermalized plasma was detected one hour after the shock, followed two hours later by a plasma piston with a bulk velocity higher than 1700 km/s. Comparison between the Prognoz and Pioneer 9 solar-wind data indicates a decrease in plasma parameters with increasing distance from the flare's central meridian.

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