Latitudinal properties of the solar wind from studies of ionic comet tails

Details Latitudinal properties of the solar wind from studies of ionic comet tails Latitudinal properties of the solar wind from studies of ionic comet tails

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ssim.conf...95b&link_type=abstract

In its Proc. of the Symp. on the Study of the Sun and Interplanetary Medium in Three Dimensions p 95-107 (SEE N76-24119 14-92)

Physics

Comets, Latitude, Solar Wind Velocity, Statistical Analysis, Variations, Polar Coordinates, Root-Mean-Square Errors, Sampling, Solar Activity, Solar Cycles

Scientific paper

A 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.

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