Thursday @ 2:30 p.m.

Coronal Magnetic Field Tools and Models III: MHD Models

Leader: Bill Abbett

This session will focus on dynamic models. We will first describe several promising techniques that allow photospheric flows and electric fields to be determined from time-sequences of magnetograms. We will then discuss the utility and efficiency of these methods, how they are validated, and how they might be included as pipeline products. Next, we will focus on the available MHD models --- their capabilities and limitations, how they are validated, and how best to incorporate these models into the suite of user tools.


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