Latitudinal distribution of solar-wind speed from magnetic observations of the sun

Details Latitudinal distribution of solar-wind speed from magnetic observations of the sun Latitudinal distribution of solar-wind speed from magnetic observations of the sun

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.347..439w&link_type=abstract

Nature (ISSN 0028-0836), vol. 347, Oct. 4, 1990, p. 439-444. Research supported by NASA and U.S. Navy.

Physics

37

Solar Corona, Solar Magnetic Field, Solar Terrestrial Interactions, Solar Wind Velocity, Sunspots, Ulysses Mission, Heliosphere, Magnetic Disturbances

Scientific paper

Empirical studies suggest a close relationship between the solar-wind speed near the earth and the magnetic structure of the solar corona. The correlation can be used to infer the latitudinal distribution of wind speed at different phases of the sunspot cycle, and to identify the sources of fast, high-latitude wind streams such as those that might be encountered by the Ulysses spacecraft on its journey toward the solar poles during 1992-1995.

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