Thermal effects of submerged horizontal flux tubes

Details Thermal effects of submerged horizontal flux tubes Thermal effects of submerged horizontal flux tubes

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308..966k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 308, Sept. 15, 1986, p. 966-974. Research supported by Harvard University.

Astronomy and Astrophysics

Astrophysics

1

Magnetic Field Configurations, Magnetic Flux, Solar Magnetic Field, Temperature Effects, Convective Heat Transfer, Horizontal Orientation, Radiative Heat Transfer

Scientific paper

Thermal effects associated with the presence of a horizontal magnetic tube in the upper convection zone of the sun are presently studied under an idealization of energy transfer as radiative-plus-convective conduction. The dark filaments with bright rims observable on the disk are predicted, and it is conjectured that this configuration leads to active regions when dynamical effects are taken into account.

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