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Brian Curtis George Mason University 11-28-2007. Global Magnetospheric Time Evolution via MHD. Community Coordinated Modeling Center (CCMC) .
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Brian Curtis George Mason University 11-28-2007 Global Magnetospheric Time Evolution via MHD.
Community Coordinated Modeling Center (CCMC) • Mission: The CCMC is a multi-agency partnership to enable, support and perform the research and development for next-generation space science and space weather models. • http://ccmc.gsfc.nasa.gov
OpenGGCM • Open Geospace General Circulation Model http://openggcm.sr.unh.edu/wiki/index.php/Grids
BATSRUS • Block Adaptive-Tree Solar-wind Roe-type Upwind Scheme
Outline • Plasma Flows • Convection • Currents • Ring Current • Cross Tail Current • Magnetopause current • 3 Model Run Movies • Features
Plasma Flows magnetopause • Flow towards sun on the inside. • flows around ionosphere • Flow away from sun • Magnetopause flow Axford and Hines model of convection
Bow Shock Magnetopause Flow towards and aroundearth
Currents • Cross Tail • Magnetopause • Ring
Cross Tail and Magnetopause Currents MagnetopauseCurrent
Model Run 1 • ESS261_CCMC_072407_1 (BATSRUS RCM)
Model Run 2 • hien_vo_111407_1 (OpenGGCM)
Model Run 3 • Natasha_Buzulukova_082907_1 (BATSRUS)
References • http://www.cs.berkeley.edu/~rajeshn/TA/cs267.sp06/hw0/results/benmar/ • http://openggcm.sr.unh.edu/wiki/index.php/Grids • http://ccmc.gsfc.nasa.gov/requests/grid_UCLA-GGCM.php • http://ccmc.gsfc.nasa.gov • Dr. Weigel (took some lecture pictures).