Interplanetary Discontinuities and Alfven Waves at High Heliographic Latitudes, Ulysses

Tsurutani, B. T.; Ho, C. M.; Arballo, J. K.; Smith, E. J.; Goldstein, B. E.; Neugebauer, M.; Balogh, A.; Feldman, W. C.

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