The Sun as a Stellar Laboratory: Unsolved Problems

Details The Sun as a Stellar Laboratory: Unsolved Problems The Sun as a Stellar Laboratory: Unsolved Problems

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219....1b&link_type=abstract

Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held

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The past decade has seen major adances in short wavelength observations of solar and stellar atmospheres. In the case of the sun SoHOYohKoh TRACE Compton GRO Granat etc and now RHESSI have provided a wealth of new data and ideas while Chandra XMM-Newton FUSE etc are taking stellar data into the precision plasma diagnostic realms already familiar to solar astronomers. Selected highlights of these results will be presented and discussed in terms of stellar/solar cross-fertilisation of ideas. Special attention will be paid to the answers and puzzles being presented by recent data from RHESSI concerning the dynamic solar atmosphere and by Chandra XMM-Newton and other data on flare stars and on hot star wind structure.

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