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Title:
Interplanetary gas. XX - Does the radial solar wind speed increase with latitude
Authors:
Brandt, J. C.; Harrington, R. S.; Roosen, R. G.
Affiliation:
AA(NASA, Goddard Space Flight Center, Laboratory for Solar Physics and Astrophysics, Greenbelt, Md.), AB(U.S. Naval Observatory, Washington, D.C.), AC(NASA, Goddard Space Flight Center, Laboratory for Solar Physics and Astrophysics, Albuquerque, N. Mex.)
Publication:
Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 1, p. 877, 878. (ApJ Homepage)
Publication Date:
03/1975
Category:
Solar Physics
Origin:
STI
NASA/STI Keywords:
ASTROMETRY, ASTRONOMICAL COORDINATES, COMET TAILS, INTERPLANETARY GAS, SOLAR WIND VELOCITY, ASTRONOMICAL MODELS, AZIMUTH, LATITUDE, RADIAL DISTRIBUTION, SPATIAL DISTRIBUTION
Comment:
A&AA ID. AAA013.074.016
DOI:
10.1086/153478
Bibliographic Code:
1975ApJ...196..877B

Abstract

The 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.

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