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Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic Storms

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dc.contributor.author Ho, C. M. en_US
dc.contributor.author Tsurutani, B. T. en_US
dc.date.accessioned 2004-09-25T23:48:31Z
dc.date.available 2004-09-25T23:48:31Z
dc.date.issued 1997
dc.identifier.clearanceno 97-0136
dc.identifier.uri http://hdl.handle.net/2014/21746
dc.description.abstract We have examined the ISEE 3 distant tail data during three intense magnetic storms and have identified the tail response to high-speed solar wind streams, interplanetary magnetic clouds, and near-Earth storms. en_US
dc.format.extent 896397 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other magnetic storms en_US
dc.title Distant Tail Behavior During High Speed Solar Wind Streams and Magnetic Storms en_US


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