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

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