Comparing Modeled EUV and X-Ray Emission from the Global Corona with Observations

Details Comparing Modeled EUV and X-Ray Emission from the Global Corona with Observations Comparing Modeled EUV and X-Ray Emission from the Global Corona with Observations

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1402m&link_type=abstract

American Astronomical Society, SPD meeting #40, #14.02; Bulletin of the American Astronomical Society, Vol. 41, p.833

Astronomy and Astrophysics

Astronomy

Scientific paper

Comparing emission in EUV and X-ray wavelengths from global coronal models provides a very sensitive constraint on coronal heating models. The ability of synthetic emission estimates to discriminate between different models increases considerably when observations are taken in many spectral lines. We will compare emission from our global 3D MHD model of the corona with EUV emission from EIT/SOHO and EUVI/SECCHI/STEREO, as well as soft X-rays from Yohkoh SXT and Hinode XRT. These constrains will help to improve our coronal heating model.
Research supported by NASA's Living With a Star Program, NASA's Heliospheric Theory Program, and NSF/CISM.

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