NTRS - NASA Technical Reports Server
An Estimate of Solar Wind Velocity Profiles in a Coronal Hole and a Coronal Streamer Area (6-40 R(radius symbol)Total electron content data obtained from the Ulysses Solar Corona Experiment (SCE) in 1991 were used to select two data sets, one associated with a coronal hole and the other with coronal streamer crossings. (This is largely equatorial data shortly after solar maximum.) The solar wind velocity profile is estimated for these areas.
Tsurutani, B. T.
Bird, M. K.
August 23, 2013
January 1, 1995
solar corona solar wind coronal streamer Ulysses