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Interplanetary Discontinuities and Alfven Waves at High Heliographic Latitudes, Ulysses

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dc.contributor.author Tsurutani, B. T. en_US
dc.contributor.author Ho, C. M. en_US
dc.contributor.author Arballo, J. K. en_US
dc.contributor.author Smith, E. J. en_US
dc.contributor.author Goldstein, B. E. en_US
dc.contributor.author Neugebauer, M. en_US
dc.contributor.author Balogh, A. en_US
dc.contributor.author Feldman, W. C. en_US
dc.date.accessioned 2004-10-03T06:05:40Z
dc.date.available 2004-10-03T06:05:40Z
dc.date.issued 1995 en_US
dc.identifier.citation Journal of Geophysical Research en_US
dc.identifier.clearanceno 95-1233
dc.identifier.uri http://hdl.handle.net/2014/31635
dc.description.abstract This paper presents results from the first statistical study of interplanetary directional discontinuities at high heliographic latitudes. Ulysses data showed that the rate of occurrence of interplanetary discontinuities (ROIDs) increased dramatically from the ecliptic plane to high (-80 degrees) heliographic latitudes. The high speed streams included Alfven waves. en_US
dc.format.extent 1009915 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other solar corona Alfven waves Ulysses en_US
dc.title Interplanetary Discontinuities and Alfven Waves at High Heliographic Latitudes, Ulysses en_US


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