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Evidence for the Reversal of Magnetic Field Polarity in Coronal Streamers

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dc.contributor.author Woo, Richard en_US
dc.date.accessioned 2004-10-01T05:55:25Z
dc.date.available 2004-10-01T05:55:25Z
dc.date.issued 1996 en_US
dc.identifier.clearanceno 96-1537 en_US
dc.identifier.uri http://hdl.handle.net/2014/27507
dc.description.abstract Faraday rotation observations are unique amongst radio occultation measurements in that they respond to magnetic field in addition to electron density, making it possible to probe the coronal magnetic field. en_US
dc.format.extent 297452 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Faraday rotation radio occultation occultation electron density pioneer 6 magnetic field polarity en_US
dc.title Evidence for the Reversal of Magnetic Field Polarity in Coronal Streamers en_US


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