Coronal sources of the intrastream structure of the solar wind

Details Coronal sources of the intrastream structure of the solar wind Coronal sources of the intrastream structure of the solar wind

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mit..reptq....s&link_type=abstract

Final Report Massachusetts Inst. of Tech., Cambridge.

Physics

Coronal Holes, Magnetic Fields, Solar Wind, Data Correlation, X Ray Telescopes

Scientific paper

Short time scale changes in the bulk speed were found not to coincide with X-ray transients near the sub-earth point nor with the number of X-ray bright points within a coronal hole and near the equator. The changes in bulk speed, it is shown, are associated with changes in light areas in a hole which may be associated with the opening or closing of magnetic field lines within the coronal hole. That there is a causal connection between these sudden changes (apperance or disappearance) in light area and sudden changes in the bulk speed of the solar wind is further evidenced by the spatial proximity on the Sun of these changing light regions to the source position of stream lines from Levine's model that connect into the same solar wind streams.

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