2.5D Simulations of Angular Momentum Transport in the Solar Interior

Details 2.5D Simulations of Angular Momentum Transport in the Solar Interior 2.5D Simulations of Angular Momentum Transport in the Solar Interior

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21621102r&link_type=abstract

American Astronomical Society, AAS Meeting #216, #211.02; Bulletin of the American Astronomical Society, Vol. 41, p.866

Astronomy and Astrophysics

Astronomy

Scientific paper

Understanding the uniform rotation of the solar radiative interior has proven quite challenging. In this talk I will briefly overview the main mechanisms proposed for this uniform rotation; internal gravity waves and magnetic fields. I will then focus on new 2.5D simulations of the coupled radiative and convective regions, which were conducted to study how angular momentum is transferred between the regions.

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