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

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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


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