Relationship between the coronal holes and high-speed streams of solar wind

Details Relationship between the coronal holes and high-speed streams of solar wind Relationship between the coronal holes and high-speed streams of solar wind

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sosyr..42...83s&link_type=abstract

Solar System Research, Volume 42, Issue 1, pp.83-89

Physics

4

96.60.Pc, Coronal Holes

Scientific paper

The relationship between two classes of coronal holes and high-speed quasi-stationary streams of solar wind at the Earth's orbit is investigated. "Open" coronal holes, whose area is invariable or increases with the height over the solar surface, are rated in the first class, and "closed" coronal holes with areas decreasing with the height are referred to as second-class holes. The parameters of the coronal holes are determined from IR and EUV images and spectroheliograms. It is shown that most open coronal holes can be associated with high-speed solar-wind streams, while most closed coronal holes exhibit a much lower correlation with such streams.

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