Modeling Coronal Jets with FLUX

Details Modeling Coronal Jets with FLUX Modeling Coronal Jets with FLUX

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp43b..01r&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP43B-01

Physics

7509 Corona, 7524 Magnetic Fields

Scientific paper

We report on a comparative study of coronal jet formation with and without reconnection using two different simulation strategies. Coronal jets are features on the solar surface that appear to have some properties in common with coronal mass ejections, but are less energetic, massive, and broad. Magnetic free energy is built up over time and then suddenly released, which accelerates plasma outward in the form of a coronal jet. We compare results from the ARMS adaptive mesh and FLUX reconnection-less codes to study the role of reconnection in this system. This is the first direct comparison between FLUX and a numerical model with a 3D spatial grid.

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