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Interplanetary gas. XX - Does the radial solar wind speed increase with latitudeThe astrometric technique used to derive solar wind speeds from ionic comet-tail orientations has been used to test the suggestion that the radial solar wind speed is higher near the solar poles than near the equator. We find no evidence for the suggested latitude variation.
Document ID
19750043159
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/153478
Authors
Brandt, J. C. (NASA Goddard Space Flight Center Laboratory for Solar Physics and Astrophysics, Greenbelt, Md., United States)
Harrington, R. S. (U.S. Naval Observatory Washington, D.C., United States)
Roosen, R. G. (NASA Goddard Space Flight Center Laboratory for Solar Physics and Astrophysics, Albuquerque, N. Mex., United States)
Date Acquired
August 8, 2013
Publication Date
March 15, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 196
Subject Category
Solar Physics
Accession Number
75A27231
Distribution Limits
Public
Copyright
Other

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