Magneto-Convection in Micropores

Details Magneto-Convection in Micropores Magneto-Convection in Micropores

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.3105b&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #31.05; Bulletin of the American Astronomical Society, Vol. 32, p.1447

Astronomy and Astrophysics

Astronomy

Scientific paper

We report results from a series of magneto-convection simulations. An initially vertical magnetic field is evolved in a 12 Mm x 12 Mm x 3 Mm solar near-surface layer at average field strengths of 0 G, 200 G and 400 G. Small dark features develop, that have sizes and lifetimes comparable to micropores observed on the solar surface. We present the properties of these micropore features, including structure, formation and evolution. This work is supported by grants from NASA and NSF.

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