The characteristics of the solar corona above the coronal hole

Details The characteristics of the solar corona above the coronal hole The characteristics of the solar corona above the coronal hole

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..797c&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Sept. 1987, p. 797-802. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Coronal Holes, Plasma Dynamics, Solar Corona, Flow Velocity, Magnetic Field Configurations, Plasma Density, Plasma Temperature

Scientific paper

A stationary self-consistent model for the formation of a corona above coronal holes with an energy source in the form of a MHD wave is considered. It is shown that more rapid (as opposed to radial) divergence of the magnetic field lines leads to a stronger cooling influence of the plasma flow on the solar corona regime. This explains the lower plasma density and temperature values and the higher flow velocity typical of coronal holes.

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