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Dawn/dusk aurora and propagating convection disturbance: ionospheric effects of high solar wind ram pressures

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dc.contributor.author Zhou, X.-Y. en_US
dc.contributor.author Tsurutani, B. T. en_US
dc.contributor.author Mende, S. B. en_US
dc.contributor.author Frey, H. U. en_US
dc.contributor.author Watermann, J. F. en_US
dc.contributor.author Sibeck, D. G. en_US
dc.contributor.author Arballo, J. K. en_US
dc.date.accessioned 2004-09-23
dc.date.available 2004-09-23
dc.date.issued 2001-04-10 en_US
dc.identifier.citation LLBL New Orleans Chapman Conference, 8/20/2001 en_US
dc.identifier.citation New Orleans, LA, USA en_US
dc.identifier.clearanceno 01-1881 en_US
dc.identifier.uri http://hdl.handle.net/2014/13196
dc.description.abstract A dawn/dusk flank auroral event has been studied using multiple observations of the WIND and POLAR spacecraft, Antarctic all-sky images and Greenland magnetometers. en_US
dc.format.extent 1493430 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other dawn/dusk aurora propagating convection disturbance ionospheric effects high solar wind ram pressuer en_US
dc.title Dawn/dusk aurora and propagating convection disturbance: ionospheric effects of high solar wind ram pressures en_US


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