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New interactive solar flare modeling and advanced radio diagnostics tools

Published online by Cambridge University Press:  08 June 2011

Gregory D. Fleishman
Affiliation:
New Jersey Institute of Technology, Newark, NJ 07102, USA Ioffe Institute, St. Petersburg 194021, Russia email: [email protected]
Gelu M. Nita
Affiliation:
New Jersey Institute of Technology, Newark, NJ 07102, USA
Dale E. Gary
Affiliation:
New Jersey Institute of Technology, Newark, NJ 07102, USA
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Abstract

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The coming years will see routine use of solar data of unprecedented spatial and spectral resolution, time cadence, and completeness in the wavelength domain. To capitalize on the soon to be available radio facilities such as the expanded OVSA, SSRT and FASR, and the challenges they present in the visualization and synthesis of the multi-frequency datasets, we propose that realistic, sophisticated 3D active region and flare modeling is timely now and will be a forefront of coronal studies over the coming years. Here we summarize our 3D modeling efforts, aimed at forward fitting of imaging spectroscopy data, and describe currently available 3D modeling tools. We also discuss plans for future generalization of our modeling tools.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011