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Solar Wind Features Responsible for Magnetic Storms and Substorms During the Declining Phase of the Solar Cycle: 197

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dc.contributor.author Tsurutani, B. en_US
dc.contributor.author Arballo, J. en_US
dc.date.accessioned 2004-10-05T05:34:29Z
dc.date.available 2004-10-05T05:34:29Z
dc.date.issued 1994-10-03 en_US
dc.identifier.citation Rikubetsu, Japan en_US
dc.identifier.clearanceno 94-1195 en_US
dc.identifier.uri http://hdl.handle.net/2014/33257
dc.description.abstract We examine interplanetary data and geomagnetic activity indices during 1974 when two long-lasting solar wind corotating streams existed. We find that only 3 major storms occurred during 1974, and all were associated with coronal mass ejections. Each high speed stream was led by a shock, so the three storms had sudden commencements. Two of the 1974 major storms were associated with shock compression of preexisting southward fields and one was caused by southward fields within a magnetic cloud. Corotating streams were responsible for recurring moderate to weak magnetic storms. en_US
dc.format.extent 478086 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other magnetospheric corotating streams solar wind en_US
dc.title Solar Wind Features Responsible for Magnetic Storms and Substorms During the Declining Phase of the Solar Cycle: 197 en_US


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