The Evolution of MHD Modeling: Coupling Local and Global Scales

Details The Evolution of MHD Modeling: Coupling Local and Global Scales The Evolution of MHD Modeling: Coupling Local and Global Scales

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh11b..02m&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH11B-02

Physics

7509 Corona, 7513 Coronal Mass Ejections, 7524 Magnetic Fields

Scientific paper

We will describe how MHD models of the solar corona and inner heliosphere have evolved over the years to include a more comprehensive coupling of local physics (on the scale of active regions and smaller length scales) with global structures (on the solar radius scale). In particular, we will discuss our efforts to understand the thermal and magnetic structure and dynamics of active regions and their coupling to the global structure of the solar corona. We will discuss initiation of CMEs that originate in active regions, and their propagation in the inner heliosphere. Research supported by NASA and the Center for Integrated Space Weather Modeling (an NSF Science and Technology Center).

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