X-ray bright points and solar wind generation.

Details X-ray bright points and solar wind generation. X-ray bright points and solar wind generation.

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp2280..221a&link_type=abstract

NASA Conf. Publ., NASA CP-2280, p. 221 - 223

Physics

Solar Coronal Holes:Solar Wind, Solar Coronal Holes:X Rays, Solar Wind:Origin, Solar Wind:Solar Coronal Holes, X Rays:Solar Coronal Holes

Scientific paper

The apparent contradiction between the fact that there is a high correlation between a high speed stream and a coronal hole and the fact that the thermal structure of the coronal hole, based on X-ray, EUV and radio observations, does not support the thermally driven solar wind models may be solved by considering that a dynamo process around X-ray bright points in a coronal hole is partly responsible in accelerating coronal plasma away from the sun.

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