Stellar/Solar Convection Simulations

Details Stellar/Solar Convection Simulations Stellar/Solar Convection Simulations

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996stin...9671199s&link_type=abstract

Technical Report, Michigan State Univ. East Lansing, MI United States

Physics

Chromosphere, Coronas, Resonant Frequencies, Solar Magnetic Field, Stellar Convection, Accretion Disks, Angular Momentum, Magnetic Fields, Oscillations, Simulation

Scientific paper

The primary objective is to understand convection in the solar envelope: its role in transporting energy and angular momentum, in generating the solar magnetic field, in providing energy to heat the solar chromosphere and corona, in exciting p-mode oscillations and in modifying their resonant frequencies. A secondary objective is to elucidate the interaction between convection, magnetic fields and shear flow in accretion disks.

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