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Connecting the Sun and the Solar Wind: I. Source Regions of the Fast Wind Observed Beyond 0.3 AU

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dc.contributor.author Woo, R. en_US
dc.contributor.author Habbal, S. en_US
dc.date.accessioned 2004-09-24T16:33:01Z
dc.date.available 2004-09-24T16:33:01Z
dc.date.issued 1999-07 en_US
dc.identifier.citation Journal of Geophysical Research en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 99-1332 en_US
dc.identifier.uri http://hdl.handle.net/2014/17882
dc.description.abstract Radio occultation and white-light measurements have shown that the solar corona comprises three distinction morphological regions in path-integrated density: streamer, quiet Sun, and polar coronal hole. en_US
dc.format.extent 1041501 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Sun Solar Wind Solar Corona en_US
dc.title Connecting the Sun and the Solar Wind: I. Source Regions of the Fast Wind Observed Beyond 0.3 AU en_US


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