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

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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


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