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| Paper: |
Using Solar Regions as Seen by Hinode XRT to Model the Coronae of Inactive Stars and Magnetic Minima |
| Volume: |
416, Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 |
| Page: |
543 |
| Authors: |
Saar, S.; Testa, P.; Weber, M.; Marsh, J. |
| Abstract: |
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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