Large-scale flows and magnetic fields in solar-like stars from global simulation with and without tachocline

Gustavo Guerrero, UFMG Federal University of Minas Gerais, Belo Horizonte, Brazil, Alexander G Kosovichev, New Jersey Institute of Technology, Center for Computational Heliophysics, Edison, NJ, United States, Piotr K Smolarkiewicz, European Centre for Medium-Range Weather Forecasts, Wokingham, United Kingdom and Elisabete M de Gouveia Dal Pino, IAG Institute of Astronomy, Geophysics and Atmospheric Sciences, Sao Paulo, Brazil
Abstract:
Back to: Linking the Solar Interior with the Corona: Observations, Models, and Data Assimilation I Posters