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| Paper: |
Solar-Stellar Connection: Relevance of YOHKOH Data |
| Volume: |
154, Cool Stars, Stellar Systems and the Sun: Tenth Cambridge Workshop |
| Page: |
1130 |
| Authors: |
Orlando, S.; Peres, G.; Reale, F.; Rosner, R.; Hudson, H. |
| Abstract: |
The similarity of late-type stars to the Sun is often assumed when studying the physical conditions in their coronae. In order to explore better such a ``solar-stellar'' connection we use the Yohkoh/SXT X-ray images to generate the distribution of the emission measure vs. temperature of the Sun and, from that, the expected emission, as it would be observed by non-solar X-ray telescopes such as ROSAT/PSPC and ASCA/SIS. We discuss the role of the various solar structures in determining the total distribution of the emission measure vs. temperature and in determining the stellar-like synthesized X-ray spectra. |
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