Solar Wind Speed Structure in the Inner Corona at 3-12R(sub)O

Woo, R.

dc.contributor.author	Woo, R.	en_US
dc.date.accessioned	2004-10-01T21:42:58Z
dc.date.available	2004-10-01T21:42:58Z
dc.date.issued	1995-05	en_US
dc.identifier.citation	EOS	en_US
dc.identifier.citation	Baltimore, MD	en_US
dc.identifier.clearanceno	95-0376	en_US
dc.identifier.uri	http://hdl.handle.net/2014/29141
dc.description.abstract	Estimates of solar wind speed obtained by Armstrong et al. [1986] based on 1983 VLA multiple-station intensity scintillation measurements inside 12 R(sub)O have been compared with white light coronagraph measurements.	en_US
dc.format.extent	26838 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	solar wind corona radio astronomy	en_US
dc.title	Solar Wind Speed Structure in the Inner Corona at 3-12R(sub)O	en_US