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Interplanetary Discontinuities in Corotating Streams and Their Interaction Regions

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dc.contributor.author Ho, C. M. en_US
dc.contributor.author Tsurutani, B. T. en_US
dc.contributor.author Sakurai, R. en_US
dc.contributor.author Goldstein, B. E. en_US
dc.contributor.author Balogh, A. en_US
dc.contributor.author Phillips, J. L. en_US
dc.date.accessioned 2004-09-30T05:48:27Z
dc.date.available 2004-09-30T05:48:27Z
dc.date.issued 1996 en_US
dc.identifier.citation Meudon, France en_US
dc.identifier.clearanceno 96-0719 en_US
dc.identifier.uri http://hdl.handle.net/2014/25222
dc.description.abstract In this study, we investigate the discontinuity properties in the low altitude corotating stream regions which are encountered during Ulyssses traveling from the south to north heliographic poles in 1995. Through the occurrence rates of directional discontinuites and tangential discontinuities, we find that there are three different regions around a high speed stream. en_US
dc.format.extent 489962 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Ulysses discontinuities rotatoinal discontinuities tangential discontinuitites RDs TDs coronal mass ejections en_US
dc.title Interplanetary Discontinuities in Corotating Streams and Their Interaction Regions en_US


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