Astronomy and Astrophysics – Astronomy
Scientific paper
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.
Marsh James
Saar Steve
Testa Paola
Weber Matthias
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