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Latitudinal properties of the solar wind from studies of ionic comet tailsA statistical analysis is presented of the orientations of ionic comet tails in the solar wind. The analysis indicates that the radial solar wind speed is not necessarily higher near the solar poles than near the equator. The results refer to a long-term, global flow pattern and do not refer to short-term variations of solar wind speed.
Document ID
19760017038
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Brandt, J. C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 8, 2013
Publication Date
March 1, 1976
Publication Information
Publication: Proc. of the Symp. on the Study of the Sun and Interplanetary Medium in Three Dimensions
Subject Category
Solar Physics
Accession Number
76N24126
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19760017031Collected WorksProceedings of the Symposium on the Study of the Sun and Interplanetary Medium in Three Dimensions19760017031Collected WorksProceedings of the Symposium on the Study of the Sun and Interplanetary Medium in Three Dimensions
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