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Дата изменения: Tue Sep 1 15:38:27 1998 Дата индексирования: Tue Oct 2 01:21:20 2012 Кодировка: Поисковые слова: molecular cloud |
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Solar and Stellar Activity: Similarities and Differences
A meeting dedicated to Brendan Byrne
Armagh 2-4th September 1998
Programme
DAY 1 - Wed. 2nd September 08:30 Registration 09:00 Introduction Mark Bailey 09:05 Brendan P. Byrne (1947-1997) Patrick Wayman Magnetic Fields in the Sun and stars: Measurements Chair: Eric Priest 09:20 Magnetic fields in the HR Diagram Jeff Linsky 10:00 The dynamic nature of the solar magnetic field Karel Schrijver 10:40 Coffee break/Posters 11:10 Review of measurements on late-type stars Jean-Francois Donati 11:50 Magnetic Activity and Variability in Stellar Coronae (EUV) Mihalis Mathioudakis 12:30 Magnetic Activity and Variability in Stellar Coronae (X-rays) Bob Stern 13:00 Lunch/Posters Magnetic Fields in the Sun and stars: Evolution Chair: Bob Stern 14:30 Evolution of chromospheric activity in low mass stars,
            as revealed through studies of open clustersSuzanne Hawley 15:15 Stellar clusters as viewed in the X-rays Robin Jeffries 16:00 Tea/Posters 16:45 Activity in pre-main sequence and very active stars Fred Walter 17:30 Finish DAY 2 - Thurs. 3rd September Physical Manifestations of Activity:
Spots, plages & prominencesChair: Marcello Rodono 09:00 Spots and Plages: The Solar Perspective Sami Solanki 09:40 Observations and modelling of starspots:
            a tool to understand stellar dynamosAntonino Lanza 10:20 New perspectives on Solar Prominences Brigitte Schmieder 11:00 Coffee/Posters 11:30 Stellar prominences (observ. + modelling) Andrew Collier Cameron 12:10 Stellar Flares (observ. + modelling) Bert van den Oord 12:50 Lunch/Posters Physical Manifestations of Activity: Flares Chair: Gordon Bromage 14:00 The Nature of flares and flare-like phenomena on the Sun Ken Phillips 14:40 Dynamic Solar Flare Model Atmospheres Bill Abbett a> 15:20 Tea 15:45 Finish 16:00 - 16:15 Tree Dedication at Armagh Observatory DAY 3 - Fri. 4th September Chromospheric and Coronal Dynamics Chair: Jeff Linsky 09:00 The Dynamical Structure of the Solar Chromosphere Rob Rutten 09:40 Theoretical chromospheric models Peter Ulmschneider 10:20 Two-Component Chromosphere Models
            for K Dwarf StarsManfred Cuntz 11:00 Coffee/Posters 11:40 Diagnostics of stellar chromospheres
            and Transition RegionsAlessandro Lanzafame Chromospheric and Coronal Dynamics Chair: Suzanne Hawley 12:30 How is the solar corona heated? Eric Priest 13:00 Lunch/Posters 14:30 X-ray coronae of stars: theory and observations Roberto Pallavicini 16:00 Tea/Posters 15:15 SOHO - where has the quiet Sun gone? Helen Mason 16:30 Activity in the Sun and late-type stars
            - similarities and differences (overall summary)Jeff Linsky 17:00 Finish
Last Revised: 25th August 1998
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