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One-parameter representation of the daily averaged solar-wind velocity
Authors:I. S. Veselovsky  I. G. Persiantsev  A. Yu. Ryazanov  Yu. S. Shugai
Affiliation:(1) Skobel’tsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119899, Russia
Abstract:An empirical formula was found to describe the dependence V(S) of the daily average solar-wind velocity V on the coronal-hole area S on the visible side of the Sun in the form of first-and second-order Taylor expansions. The results can be used for approximate evaluation of the solar-wind velocity at the Earth’s orbit from coronal-hole observations.
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