Interplanetary scintillation and flare - Produced disturbances

Details Interplanetary scintillation and flare - Produced disturbances Interplanetary scintillation and flare - Produced disturbances

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasau...2..378w&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 9th, Parkes, New South Wales, Australia, May 14-16, 1975.) Astronomi

Astronomy and Astrophysics

Astronomy

2

Interplanetary Medium, Solar Activity Effects, Solar Flares, Diurnal Variations, Luminous Intensity, Power Spectra, Satellite Observation, Scintillation, Shock Wave Propagation, Solar Radio Bursts, Type 2 Bursts

Scientific paper

The properties of 5 large scale flare-produced disturbances in the interplanetary medium have been determined by combining scintillation and spacecraft data. The average shape of the disturbances, inferred by model-fitting to a range of disturbance geometries and including the approximate arrival time of the shock at widely separated spacecraft, is consistent with the models of de Young and Hundhausen (1971) in which plasma is initially injected into a cone of half-angle between 30 and 60 deg and subsequently undergoes transverse expansion as it moves away from the sun. Each of the events is related to a specific active region on the sun.

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