Stationary siphon flows in thin magnetic flux tubes

Details Stationary siphon flows in thin magnetic flux tubes Stationary siphon flows in thin magnetic flux tubes

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...222..297d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 222, no. 1-2, Sept. 1989, p. 297-306.

Astronomy and Astrophysics

Astrophysics

48

Magnetic Flux, Siphoning, Solar Atmosphere, Solar Magnetic Field, Coronal Loops, Critical Flow, Field Strength, Magnetohydrodynamics, Shock Tubes

Scientific paper

A self-consistent calculation of a siphon flow in isolated magnetic flux tubes, together with a large-scale mechanical equilibrium of the tube, is carried out. The relevant equations for the problem and the model atmosphere being used are presented, some qualitative aspects about stationary flows are deduced, and the behavior of critical flow is also considered. Finally, an interpretation of the calculations to solar application is discussed.

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