The dynamics of fibril magnetic fields. I - Effect of flux tubes on convection.

Details The dynamics of fibril magnetic fields. I - Effect of flux tubes on convection. The dynamics of fibril magnetic fields. I - Effect of flux tubes on convection.

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...256..292p&link_type=abstract

Astrophysical Journal, Part 1, vol. 256, May 1, 1982, p. 292-302.

Astronomy and Astrophysics

Astrophysics

26

Magnetic Flux, Solar Atmosphere, Solar Magnetic Field, Convective Flow, Energy Dissipation, Reynolds Number, Topology

Scientific paper

Observations have established the general fibril state of the magnetic field at the visible surface of the sun. This extraordinary state of the field, in separate intense flux tubes, implies that the convection has a relatively permanent, closed topology, in spite of the large Reynolds number. This paper explores some of the effects of the separate flux tubes on the convective motions, generally pushing the convective cells toward aligning their downdrafts with the flux tubes so as to minimize the dissipation.

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