Constraints on angular momentum transport in the Sun from simulations of the tachocline

Details Constraints on angular momentum transport in the Sun from simulations of the tachocline Constraints on angular momentum transport in the Sun from simulations of the tachocline

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007an....328.1146g&link_type=abstract

Astronomische Nachrichten, Vol.328, Issue 10, p.1146

Astronomy and Astrophysics

Astronomy

Sun: Interior, Sun: Magnetic Fields, Sun: Rotation

Scientific paper

I present a new numerical tool for studying the interaction of meridional flows and magnetic fields, and study their role in establishing angular-momentum balance in the solar radiative zone. Quantitative comparisons with helioseismic observations provide stringent constraints on existing models of the dynamics of the solar interior.

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