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

Woo, R.; Habbal,   S.

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