New interactive solar flare modeling and advanced radio diagnostics tools

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

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.

Original languageEnglish (US)
Title of host publicationAdvances in Plasma Astrophysics
EditorsAlfio Bonanno, Elisabete de Gouveia Dal Pino, Alexander Kosovichev
Pages280-283
Number of pages4
EditionS274
DOIs
StatePublished - Sep 2010

Publication series

NameProceedings of the International Astronomical Union
NumberS274
Volume6
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

All Science Journal Classification (ASJC) codes

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Keywords

  • Sun: corona
  • Sun: flares
  • Sun: magnetic fields
  • Sun: radio radiation
  • methods: numerical
  • radiation mechanisms: non-thermal
  • stars: flares

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