The flare-CME relationship – determining factors (if any!) Sarah Matthews, Lucie Green, Hilary Magee, Louise Harra & Len Culhane MSSL, University College.
SPACE NEWS
1 An Overview of LH Transition and Future Perspectives Hogun Jhang WCI Center for Fusion Theory, NFRI, Korea Asia-Pacific Transport Working Group (APTWG.
Modeling the Dynamic Evolution of the Solar Atmosphere: C4: HMI-AIA Team Meeting: 2-14-06 Bill Abbett SSL, UC Berkeley.
Photospheric Sources of Very Fast (>1100km/s) Coronal Mass Ejections Recent studies show that only very fast CMEs (> 1100 km/s) are capable of producing.
Nonlinear Extended MHD Simulation Using High-Order Finite Elements C. Sovinec, C. Kim, H. Tian, Univ. of WI-Madison D. Schnack, A. Pankin, Science Apps.
Can we use nonlinear and selfconsistent models for data analysis? We learned from Prof. Schindler about the importance of nonlinear and selfconsistent.
CROSS-SCALE and SCOPE: The future in Space Plasma Physics Matt Taylor on behalf of Steve Schwartz, Masaki Fujimoto and the Cross-Scale and SCOPE Teams.
SHINE SEP Campaign Events: Detailed comparison of active regions AR9906 and AR0069 in the build-up to the SEP events of 21 Apr 2002 and 24 Aug 2002 D.
1 Status of Physics and Configuration Studies of ARIES-CS T.K. Mau University of California, San Diego L.P. Ku, PPPL J.F. Lyon, ORNL P.R. Garabedian, CIMS/NYU.
Structure, Equilibrium and Pinching of Coronal Magnetic Fields Slava Titov SAIC, San Diego, USA Seminar at the workshop „Magnetic reconnection theory“
Three-Dimensional Reconstruction of AR 11158 During its Emergence Phase Using SDO/HMI Observations Georgios Chintzoglou*, Jie Zhang School of Physics,
