Testing coronal plasma diagnostics using 3D MHD models of the solar atmosphere

Details Testing coronal plasma diagnostics using 3D MHD models of the solar atmosphere Testing coronal plasma diagnostics using 3D MHD models of the solar atmosphere

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh53c..06t&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH53C-06

Astronomy and Astrophysics

Astrophysics

[7500] Solar Physics, Astrophysics, And Astronomy, [7509] Solar Physics, Astrophysics, And Astronomy / Corona, [7549] Solar Physics, Astrophysics, And Astronomy / Ultraviolet Emissions

Scientific paper

We synthesize coronal images and spectra from advanced 3D radiative MHD simulations obtained from the state-of-the-art Bifrost code, and explore how well they reproduce coronal observations with SDO/AIA and Hinode/EIS and XRT. We apply standard diagnostic techniques (e.g., density, temperature, abundance diagnostics) to the synthetic observations and investigate how accurately the derived physical information matches the plasma parameters of the model. We discuss the limitations of the diagnostics and their implications.

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