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Intermittent Turbulence in Solar Wind from the South Polar Hole

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dc.contributor.author Ruzmaikin, A. en_US
dc.contributor.author Feynman, J. en_US
dc.contributor.author Goldstein, B. en_US
dc.contributor.author Smith, E. en_US
dc.contributor.author Balogh, A. en_US
dc.date.accessioned 2004-10-05T05:13:23Z
dc.date.available 2004-10-05T05:13:23Z
dc.date.issued 1994
dc.identifier.citation Journal of Geophysical Research en_US
dc.identifier.clearanceno 94-1058
dc.identifier.uri http://hdl.handle.net/2014/33124
dc.description.abstract The magnetic fields measured by the Ulyses spacecraft are used to study solar wind turbulence in the fast solar wind from the south polar hole. en_US
dc.format.extent 958126 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other components of the magnetic fields non-Gaussian effects of intermittency solar wind turbulence solar wind en_US
dc.title Intermittent Turbulence in Solar Wind from the South Polar Hole en_US


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