Physics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...75..347m&link_type=abstract
Solar Physics, vol. 75, Jan. 1982, p. 347-350.
Physics
23
Coronal Holes, Magnetic Field Configurations, Solar Physics, Stellar Mass Ejection, Bubbles, Magnetohydrodynamic Flow, Plumes, Solar Wind
Scientific paper
A nonthermal mechanism for driving coronal hole mass loss is proposed. Three empirical results are noted, namely (1) that polar plumes with short-lived X-ray bright points (XBP) at their base are sites of matter flow sufficient to account for the total solar mass flux, (2) that solar wind densities are positively correlated with the number of XBP in coronal holes, and (3) that XBP are associated with newly emerged magnetic flux. It is noted that since the dynamical development following the onset of nonequilibrium is a hitherto unsolved problem, subsequent features in the scenario described here are relatively speculative. It is proposed that bubbles of matter ejected from magnetic reconnection sites in polar plumes drive the solar wind in coronal holes.
Ahmad Imad Aldean
Mullan Dermott J.
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