The physical interpretation of Alfven wave flux in the solar corona

Details The physical interpretation of Alfven wave flux in the solar corona The physical interpretation of Alfven wave flux in the solar corona

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194..381h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Feb. 1981, p. 381, 382.

Astronomy and Astrophysics

Astronomy

2

Magnetohydrodynamic Waves, Solar Corona, Solar Wind, Conservation Equations, Magnetohydrodynamic Flow, Wave Propagation

Scientific paper

A recent analysis of coronal hole acceleration by McWhirter and Kopp
(1979) is examined. It is shown that the approach adopted by these
authors is invalid on physical grounds.

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