Large solar wind disturbances during late May and early June 1991

Details Large solar wind disturbances during late May and early June 1991 Large solar wind disturbances during late May and early June 1991

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..160..363m&link_type=abstract

Solar Physics, Volume 160, Issue 2, pp.363-370

Physics

1

Scientific paper

Solar wind data from the Ames experiment aboard the Pioneer Venus Orbiter, coincident with a period of unprecedented solar activity that began at the end of May, 1991, within the highly active earlier portion of 1991, are summarized and discussed. Some comparison is made with corresponding data from Earth. Some particularly large, strong shocks and solar ejecta were observed at Venus. The solar longitude of Venus, relative to associated flares, varied over a wide range, for a series of flares that produced X-rays that saturated the GOES X-ray counters. Some of the disturbances at Venus must be due to CMEs with longitudinal extents up to ˜40 50 deg.

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