The Solar Magnetic Field and the Solar Wind: Existence of Preferred Longitudes

Neugebauer, M.; Smith, E.; Ruzmaikin, A.; Feynman, J.; Vaughan, A.

dc.contributor.author	Neugebauer, M.	en_US
dc.contributor.author	Smith, E.	en_US
dc.contributor.author	Ruzmaikin, A.	en_US
dc.contributor.author	Feynman, J.	en_US
dc.contributor.author	Vaughan, A.	en_US
dc.date.accessioned	2004-09-24T16:44:28Z
dc.date.available	2004-09-24T16:44:28Z
dc.date.issued	1999-08	en_US
dc.identifier.citation	Journal of Geophysical Research	en_US
dc.identifier.citation	USA	en_US
dc.identifier.clearanceno	99-1455	en_US
dc.identifier.uri	http://hdl.handle.net/2014/18001
dc.description.abstract	Direct measurements of the solar wind and the interplanetary magnetic field acquired over more than three solar cycles both near Earth and in interplanetary space are used to search for signatures of a persistent dependence of solar wind properties on solar longitude.	en_US
dc.format.extent	1236803 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	solar magnetic field solar wind	en_US
dc.title	The Solar Magnetic Field and the Solar Wind: Existence of Preferred Longitudes	en_US