Using Solar Regions as Seen by Hinode XRT to Model the Coronae of Inactive Stars and Magnetic Minima

Details Using Solar Regions as Seen by Hinode XRT to Model the Coronae of Inactive Stars and Magnetic Minima Using Solar Regions as Seen by Hinode XRT to Model the Coronae of Inactive Stars and Magnetic Minima

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..543s&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

Astronomy and Astrophysics

Astronomy

Scientific paper

We use carefully calibrated, multi-filter X-ray data from Hinode XRT to compute differential emission measures (DEM) for spatially averaged, less active solar features (coronal holes, quiet Sun, X-ray bright points). We use linear combinations of these regions to construct model quiet coronae for comparison with inactive stars, specifically, stars which may be in Maunder-like magnetic minima. In this way, test how well a mix of existing solar features can be used to model conditions in magnetic minima.

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