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Mass Flux in the Ecliptic Plane and Near the Sun Deduced from Doppler ScintillationIn this paper, we use Doppler scintillation measurements to investigate mass flux of these two types of solar wind inside 0.3AU, where in-situ measurements have not been possible.
Document ID
20210004122
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
hdl:2014/32416
Authors
Gazis, Paul R.
Woo, Richard
Date Acquired
January 1, 1994
Publication Date
January 1, 1994
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
solar
winds
doppler
scintillation
doppler
radar
solar
cycle
mass
flux

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