Physics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mcch.conf..137y&link_type=abstract
International Conference on Mechanisms of Chromospheric and Coronal Heating, p. 137 - 139
Physics
Scientific paper
The author examines the energetics of a solar coronal hole in the
framework of magnetohydrodynamics. Given typical values of the observed
parameters, it is estimatet that the Poynting flux maintained by the
solar rotation and a trailing magnetic field is potentially capable of
driving and heating a wind stream in a coronal hole region.
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