Solar wind disturbances in the outer heliosphere, caused by six successive solar flares from the same active region

Details Solar wind disturbances in the outer heliosphere, caused by six successive solar flares from the same active region Solar wind disturbances in the outer heliosphere, caused by six successive solar flares from the same active region

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983georl..10..577a&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 10, July 1983, p. 577-579.

Other

8

Heliosphere, Shock Wave Interaction, Solar Flares, Solar Wind, Disturbances, Galactic Cosmic Rays, Solar Activity Effects

Scientific paper

Solar wind disturbances caused by six hypothetical flares from the same active region are traced out to about 15 au, using a simple, empirical modeling method developed by Hakamada and Akasofu (1982). The method provides a first order construction, temporal and spatial, of flare-induced shocks and their multiple interactions with each other, as well as with the corotating interaction regions. The results are discussed in connection with recent cosmic ray observations by space probes.

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