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 |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en_US |
|
dc.subject.other |
Solar Flares |
en_US |
dc.title |
Terrestrial Response to Eruptive Solar Flares: Geomagnetic Storms |
en_US |