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Ka-band and X-band observations of the solar corona aquired during the Cassini 2002 superior conjunctionA superior solar conjunction occurs when the sun lies near the signal path of a source as observed from the Earth. Interplanetary spacecraft sent to the planets typically encounter one or more solar conjunctions during their mission lifetimes. During these periods, the signals sent to and from the spacecraft encounter degradation due to the intervening charged particles of the solar corona.
Document ID
20060030172
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Morabito, D. D.
Date Acquired
August 23, 2013
Publication Date
September 25, 2002
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
propagation Ka-band solar corona solar plasma

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