Sunspot Model Atmosphere from Inversion of Stokes Profiles

Details Sunspot Model Atmosphere from Inversion of Stokes Profiles Sunspot Model Atmosphere from Inversion of Stokes Profiles

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.24w&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

We present results of a spectropolarimetric analysis of sunspots. By inversion of full Stokes spectra observed in serveral spectral regions in the optical at the THEMIS facility we infer the height dependence of physical quantities such as the temperature, LOS velocity and magnetic field for different sunspot regions. The wide spectral range and the use of TiO and MgH transitions, which are extremely temperature sensitive and can be treated in LTE even in higher layers, allow us to extend and improve a sunspot model atmosphere.

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