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Extension of Coronal Structure Into Interplanetary SpaceThe evolution of the solar corona and its imprint on the solar wind is investigated by comparing Ulysses radio occultation measurements of path-integrated electron density and density fluctuations in the heliocentric distance range of 21-32R(sub o) with simultaneous measurements of the solasr corona by the HAO Mauna Loa K-coronameter.
Document ID
20060036833
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/27743
Authors
Woo, Richard
Habbal, Shadia Rifai
Date Acquired
August 23, 2013
Publication Date
January 1, 1996
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
solar corona corona radio occultation Ulysses

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