Physics
Scientific paper
Jul 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...43..237r&link_type=abstract
Solar Physics, vol. 43, July 1975, p. 237-247.
Physics
5
Geomagnetism, Interplanetary Medium, Plasma Turbulence, Scintillation, Solar Flares, Solar Wind, Magnetic Measurement, Satellite Observation, Solar Wind Velocity, Time Series Analysis
Scientific paper
From interplanetary-scintillation (IPS) and spacecraft measurements of the solar wind combined with geomagnetic observations, the passage of three main disturbances through the solar wind from solar flares on August 2, 4 and 7 is identified. From a detailed study of the IPS data covering the third event, it is concluded that the extent of the disturbance front at 1 AU covered about plus or minus 60 deg in longitude and more than 30 deg in latitude from the flare normal. If interpreted as a blast wave according to the model of De Young and Hundhausen (1971), the disturbance was ejected from the sun into a cone of half-angle 45 deg plus or minus 15 deg.
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