Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.125..375p&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 125, no. 2, Aug. 1986, p. 375-378.
Astronomy and Astrophysics
Astrophysics
Cloud Chambers, Plasma Clouds, Shock Waves, Solar Flares, Helium Plasma, Shock Fronts, Solar Corona
Scientific paper
A mechanism explaining the generation of the 'helium-enriched plasma-condensation cloud' (HAE-events) behind the front of shock waves associated with mass-ejecting flares is presented. The mechanism is based on the occurrence of physical conditions, analogous to those in a Wilson cloud chamber in a magnetic field, behind the front of a flare-generated shock wave propagation out into interplanetary space. Consequently, if the solar atmosphere above the flare active region is saturated with ejected helium plasma, conditions are created for the forming of the 'helium-enriched plasma-condensation cloud' in the temperature-depressed region behind the shock wave front.
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