LYOT, SFSA, Juillet 20071 LYOT : LYman Orbiting Telescopes à bord de la mission franco-chinoise SMESE (Small Explorer for solar Erupions) Frédéric Auchère,
A complete study of magnetic flux emergence, interaction, and diffusion should take into account some “anomalies” In the photosphere we can observe flux.
Evolution of Magnetic Helicity in the Corona During Flux Emergence Anna Malanushenko, Humed Yusuf, Dana Longcope.
SHINE Campaign Event: 1-2 May 1998 Brian Welsch (& Yan Li) Space Sciences Laboratory, UC Berkeley Introduction: Data, Context, etc. Work: Completed & Ongoing.
THE FORMATION OF FILAMENT CHANNELS K. Muglach, Y.-M. Wang Naval Research Laboratory.
Coronal Heating of an Active Region Observed by XRT on May 5, 2010 A Look at Quasi-static vs Alfven Wave Heating of Coronal Loops Amanda Persichetti Aad.
Penumbral-like Structures in the Photosphere as a Manifestation of Flux Emergence
1 Introduction: Onset of solar flares and coronal mass ejections Yokoyama, T. Dept. Earth & Planetary Science, University of Tokyo Isobe, H. Univ. Tokyo.
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Solar seminor: 4 Oct. 2004 (1)Eruption of a multiple-turn helical magnetic flux tube in a large flare : Evidence for external and i ternal reconnection.
ITP 2008 [email protected] MRI Driven turbulence and dynamo action Fausto Cattaneo University of Chicago Argonne National Laboratory.
Observations of Filament Channels by Hinode/XRT and STEREO
