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Connecting the Sun and the solar wind: source regions of the fast wind observed in interplanetary space

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dc.contributor.author Woo, R. en_US
dc.contributor.author Habbal, S. en_US
dc.date.accessioned 2004-09-23T17:34:11Z
dc.date.available 2004-09-23T17:34:11Z
dc.date.issued 2000-06-01 en_US
dc.identifier.citation Journal of geophysical research, Vol. 105, No. A6, 2000, pp. 12667-12674 en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 00-0313 en_US
dc.identifier.uri http://hdl.handle.net/2014/13936
dc.description.abstract Highly sensitive radio occultation and white light measurements of path-integrated density have shown that the solar corona comprises three distinct morphological regions, streamer, quiet Sun, and polar coronal hole, which except for the streamer region, extend radially into interplanetary space from 1.15 R***s*** to at least 30 R***s***. The authors build on these results by comparing solar wind flow speeds observed at the same time as path-integrated density. en_US
dc.format.extent 2000896 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other solar corona solar wind en_US
dc.title Connecting the Sun and the solar wind: source regions of the fast wind observed in interplanetary space en_US


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