Computer Science
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..549b&link_type=abstract
Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 549
Computer Science
Solar Wind Plasma, Sources Of Solar Wind, Planetary Bow Shocks, Interplanetary Shocks
Scientific paper
Coronal holes are the sources of the solar wind and, according to recent YOHKOH observations, may undergo rapid changes in association with explosive solar activity. Rapid changes in a hole's structure will produce rapid changes in the characteristics of the wind emerging from it and, in the particular case of a sudden enlargement of the hole's base, a sudden increase in the wind velocity can be produced which will lead to the formation of an interplanetary shock. We discuss the characteristics of shocks formed in such a way and compare them with the observed characteristics of shocks in interplanetary space.
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