Observations on Current Sheet and Magnetic Reconnection in Solar Flares Haimin Wang and Jiong Qiu BBSO/NJIT.
TOWARDS A REALISTIC, DATA-DRIVEN THERMODYNAMIC MHD MODEL OF THE GLOBAL SOLAR CORONA Cooper Downs, Ilia I. Roussev, Bart van der Holst, Noe Lugaz, Igor.
WG4 Multi-wavelength Correlative Studies Group Members Marina BATTAGLIA Cristina CHIFOR Brian DENNIS Martin FIVIAN Lyndsay FLETCHER Iain HANNAH Hugh HUDSON.
Elmau III, March 16, 2004 Coronal mass ejections A critical view of interpretations H.S. Hudson (UC Berkeley)
Modeling Emerging Magnetic Flux W.P. Abbett, G.H. Fisher & Y. Fan.
A Simplified Treatment of Optically Thick Radiative Transfer in Large-scale Convection Zone to Corona Models W.P. Abbett and G.H. Fisher Space Sciences.
Three-dimensional MHD simulations of emerging flux and associated magnetic reconnection Hiroaki Isobe (DAMTP, Cambridge / Tokyo) Takehiro Miyagoshi, Kazunari.
3D Heliospheric Reconstructions from the SECCHI White Light Coronagraphs Onboard STEREO: Overview of the NRL Approach J. Newmark, J. Cook, P. Reiser, P.
Update of the French activities relevant to ILWS Jean-Yves Prado, CNES.
Coronal hard X-ray sources and associated decimetric/metric radio emissions N. Vilmer D. Koutroumpa (Observatoire de Paris- LESIA) S.R Kane G. Hurford.
195 Å image – behind 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – ahead SECCHI Extreme.
On mass evolution of CMEs
