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Heliomagnetic Latitude Dependence of Heliospheric Magnetic Field

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dc.contributor.author Burton, M. en_US
dc.contributor.author Smith, E. en_US
dc.contributor.author Balogh, A. en_US
dc.contributor.author Murphy, N. en_US
dc.date.accessioned 2004-10-03T06:05:25Z
dc.date.available 2004-10-03T06:05:25Z
dc.date.issued 1995
dc.identifier.citation JPL and LANL meeting on Solar Wind en_US
dc.identifier.citation Dana Pt., CA en_US
dc.identifier.clearanceno 95-1231
dc.identifier.uri http://hdl.handle.net/2014/31633
dc.description.abstract ICE and IMP-8 magnetic field data from 1984 1988 were analyzed in a magnetic coordinate system defined by the orientation of the solar magnetic dipole. The heliomagnetic latitude dependence of the radial component of the magnetic field (Br) was then investigated in the range of magnetic latitudes from 60 above and below the heliospheric current sheet. Investigators found that Br reverses sign abruptly across the current sheet, consistent with solar magnetic field models, but inconsistent with the source surface models. en_US
dc.format.extent 953154 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other ICE IMP-8 magnetic field data solar magnetic dipole heliomagnetic latitude dependence heliospheric current sheet en_US
dc.title Heliomagnetic Latitude Dependence of Heliospheric Magnetic Field en_US


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