Dynamics of anchored flux tubes in the convection zone. I - Details of the model

Details Dynamics of anchored flux tubes in the convection zone. I - Details of the model Dynamics of anchored flux tubes in the convection zone. I - Details of the model

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...341..533c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 341, June 1, 1989, p. 533-548. Sponsorship: National Science Council of the

Astronomy and Astrophysics

Astrophysics

46

Convection, Magnetic Flux, Solar Interior, Solar Magnetic Field, Convective Heat Transfer, Equations Of Motion, Magnetohydrodynamic Stability, Photosphere

Scientific paper

A model for the emergence of buoyant segments of magnetic flux tubes whose ends are still anchored in the stable layers below the convection zone is developed. This model is based on the thin flux tube approximation of Spruit. Several specific examples of buoyant flux tube evolution computed with the model are described. In particular, attention is given to an example of a flux tube which results in upflows as it emerges, in contrast to the downflows generally believed to accompany the Parker instability.

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