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Scintillation effects on radio wave propagation through solar corona

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dc.contributor.author Ho, C. M. en_US
dc.contributor.author Sue, M. K. en_US
dc.contributor.author Bedrossian, A. en_US
dc.contributor.author Sniffin, R. W. en_US
dc.date.accessioned 2004-09-17T05:10:29Z
dc.date.available 2004-09-17T05:10:29Z
dc.date.issued 2002-08-18 en_US
dc.identifier.citation 27th URSZ General Meeting en_US
dc.identifier.citation Maastricht, Netherlands en_US
dc.identifier.clearanceno 02-1034 en_US
dc.identifier.uri http://hdl.handle.net/2014/8532
dc.description.abstract When RF waves pass through the solar corona and solar wind regions close to the Sun, strong scintillation effects appear at their amplitude, frequency and phase, especially in the regions very close to the Sun (less than 4 solar radius). en_US
dc.format.extent 2917998 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other solar corona solar wind propagation scintillation degradation en_US
dc.title Scintillation effects on radio wave propagation through solar corona en_US


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