Near Surface Magneto-Convection

Details Near Surface Magneto-Convection Near Surface Magneto-Convection

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.5501b&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #55.01; Bulletin of the American Astronomical Society, Vol. 31, p.909

Astronomy and Astrophysics

Astronomy

Scientific paper

The emergence of magnetic flux alters the structure of the solar surface. We use simulations of magneto-convection of a near surface layer to investigate the dynamical interaction between magnetic fields and convection. The results of these simulations are presented to show the behavior of emerging flux tubes as well as the three dimensional structure and evolution of bright points and small pores.

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