Incorporating Magnetogram Data into Time-Dependent Coronal Field Models

Details Incorporating Magnetogram Data into Time-Dependent Coronal Field Models Incorporating Magnetogram Data into Time-Dependent Coronal Field Models

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm51a1340f&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SM51A-1340

Astronomy and Astrophysics

Astrophysics

[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7519] Solar Physics, Astrophysics, And Astronomy / Flares, [7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields

Scientific paper

We briefly review our efforts to incorporate sequences of photospheric
vector magnetograms into MHD simulations of coronal evolution, in an
effort to create data-driven models of the coronal magnetic field. Such
models should improve our understanding of flares and coronal mass
ejections (CMEs), and might eventually lead to predictive capabilities.

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