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Scintillation effects on radio wave propagation through solar coronaWhen 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).
Document ID
20060029492
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Ho, C. M.
Sue, M. K.
Bedrossian, A.
Sniffin, R. W.
Date Acquired
August 23, 2013
Publication Date
August 18, 2002
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
solar corona solar wind propagation scintillation degradation

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