A cause of the solar wind speed variations - an update

Details A cause of the solar wind speed variations - an update A cause of the solar wind speed variations - an update

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89..357h&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, Jan. 1, 1984, p. 357-361.

Physics

19

Periodic Variations, Solar Terrestrial Interactions, Solar Wind Velocity, Distance, Latitude, Photosphere, Solar Magnetic Field

Scientific paper

The dependence of the solar-wind speed (V) on the heliographic latitude is investigated on the basis of published satellite observations from the period May 1976-August 1977. The relationship of V (in km/sec) to the latitudinal angular distance (lambda) of the earth from the magnetic neutral line (computed from observed photospheric magnetic fields) is found to be V = 408 + 473 sin sq lambda during the period analyzed. No dependence of V on the heliographic latitude of the earth is detected. Tables and graphs of the data are provided.

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