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Terrestrial Response to Eruptive Solar Flares: Geomagnetic Storms

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dc.contributor.author Tsurutani, Bruce T. en_US
dc.date.accessioned 2004-10-03T03:42:29Z
dc.date.available 2004-10-03T03:42:29Z
dc.date.issued 1995-04 en_US
dc.identifier.citation American Institute of Physics en_US
dc.identifier.clearanceno 95-0770 en_US
dc.identifier.uri http://hdl.handle.net/2014/30902
dc.description.abstract During the interval of August 1979 - December 1979, 56 unambiguous fast forward shocks were identified using magnetic field and plasma data collected by the ISEE-3 spacecraft. Because this interval is a solar maximum we assume the streams causing these shocks are associated with coronal mass ejections and eruptive solar flares. For these shocks we shall describe the shock-storm relationship for the level of intense storms (Dst < -100 nT). Then, we will discuss the interplanetary structures that are associated with the large-amplitude and long-duration negative Bz fields, which are found in the sheath field and/or driver gas regions of the shock and are thought to be the main cause of the intense storms. en_US
dc.format.extent 762872 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Solar Flares en_US
dc.title Terrestrial Response to Eruptive Solar Flares: Geomagnetic Storms en_US


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