Effect of areal expansion and coronal heating on the solar wind

Details Effect of areal expansion and coronal heating on the solar wind Effect of areal expansion and coronal heating on the solar wind

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..387w&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 387-390

Physics

Solar Physics, Solar Corona, Solar Wind

Scientific paper

Empirical studies have shown that the solar wind speed at Earth is inversely correlated with the areal expansion rate of magnetic flux tubes near the Sun. Recent model calculations that include a self-consistent determination of the coronal temperature allow one to understand the physical basis of this relationship; they also suggest why the solar wind mass flux is relatively constant.

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