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Extension of the Polar Coronal Hole Boundary into Interplanetary Space

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dc.contributor.author Woo, R. en_US
dc.contributor.author Habbal, S. R. en_US
dc.contributor.author Howard, R. A. en_US
dc.contributor.author Korendyke, C. M. en_US
dc.date.accessioned 2004-09-24T20:58:21Z
dc.date.available 2004-09-24T20:58:21Z
dc.date.issued 1998-04 en_US
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-0860 en_US
dc.identifier.uri http://hdl.handle.net/2014/19466
dc.description.abstract White-light measurements made by the Mk III Mauna Loa K-coronameter and the SOHO LASCO C2 and C3 coronagraphs, extending from 1.15 to 30 Ro, have been combined to show that the boundaries of polar coronal holes, as determined by measurements of path-integrated density, extend approximately radially into interplanetery space. en_US
dc.format.extent 1383884 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other polar coronal radio occultation en_US
dc.title Extension of the Polar Coronal Hole Boundary into Interplanetary Space en_US


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