The International Heliophysical Year and Universal Processes In Space Science Acknowledgments: Crooker, Davila, Fuller-Rowell, Gopalswamy, Onsager, Siscoe,
The flare-CME relationship – determining factors (if any!) Sarah Matthews, Lucie Green, Hilary Magee, Louise Harra & Len Culhane MSSL, University College.
COSMIC MAGNETIC FIELDS ElisaBete M. de Gouveia Dal Pino IAG-USP UFRRJ, October 2005.
P.K. Manoharan Radio Astronomy Centre National Centre for Radio Astrophysics Tata Institute of Fundamental Research Ooty 643001, India [email protected].
EUV filaments in 3D from magnetic extrapolations toward stereoscopic observations G. Aulanier & B. Schmieder Observatoire de Paris, LESIA.
European and French solar physics from space Jean ARNAUD Laboratoire FIZEAU Observatoire de la côte d’Azur Université de Nice Sophia Antipolis.
Using Potential Field Models to Learn About CME Coronal Context and Consequences J.G. Luhmann and Yan Li (Space Sciences Lab, UCB) C.N. Arge (CIRES, U.
U.W., April 14, 2005 Solar flares in the new millennium H.S. Hudson SSL/UCB.
Group V: Report Regular Members: K. Arzner, A. Benz, C. Dauphin, G. Emslie, M. Onofri, N. Vilmer, L. Vlahos Visitors: E. Kontar, G. Mann, R. Lin, V. Zharkova.
January 30 2006Nobeyama radioheliograph visit Microwave Signatures of Fast CMEs Nat Gopalswamy NASA Goddard Space Flight Center Greenbelt MD 20771 USA.
