Comparison with Observations of EUV and X-Ray Emissions Calculated with Different Heating Models for Active Region 7986

Details Comparison with Observations of EUV and X-Ray Emissions Calculated with Different Heating Models for Active Region 7986 Comparison with Observations of EUV and X-Ray Emissions Calculated with Different Heating Models for Active Region 7986

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp31a..03l&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP31A-03

Physics

7509 Corona, 7538 Solar Irradiance, 7549 Ultraviolet Emissions

Scientific paper

We have calculated the EUV and X-Ray emissions for AR 7986 in late August 1996 for different heating models using three-dimensional simulations of the magnetic field and of the thermal structure. From our simulations we have extracted time-sequences of emissions from different point of views and compared them quantitatively with the observations from SoHo EIT and Yohkoh SXT. Work supported by NASA LWS program.

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