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Transients and Mass Ejections Observed in Radio Occultation Measurements of the Solar CoronaA wide variety of radio propagation and scattering phenomena observed when a radio source is occulted by the solar corona has formed the basis for probing the solar corona for over four decades.
Document ID
20060041704
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/21951
Authors
Woo, R.
Date Acquired
August 23, 2013
Publication Date
January 1, 1997
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
solar corona radio sources

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