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 |