Coronal Modeling: Present Status and Challenges for the Future*

Details Coronal Modeling: Present Status and Challenges for the Future* Coronal Modeling: Present Status and Challenges for the Future*

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agusmsh22a..04l&link_type=abstract

American Geophysical Union, Spring Meeting 2009, abstract #SH22A-04

Physics

7509 Corona, 7511 Coronal Holes, 7513 Coronal Mass Ejections (2101), 7524 Magnetic Fields

Scientific paper

The solar corona strongly influences space weather at Earth, via eruptive phenomena such as coronal mass ejections, and through its structure, which leads to the formation of fast solar wind streams that trigger recurrent geomagnetic activity. MHD models that address both the dynamics and structure of the solar corona have advanced considerably in recent years, but many challenges remain if these models are to provide reliable space weather forecasting tools. In this talk we describe these challenges and the prospects for meeting them. *Research supported by NASA, NSF and AFOSR.

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