Active Region Evolution and the Removal of Magnetic Helicity by CMEs Len Culhane Mullard Space Science Laboratory University College London.
Imaging Solar Coronal Structure With TRACE Leon Golub, SAO TRACE: ISAS - 4 Feb. 2003.
Photospheric Flows and Magnetic Fields, and Their Role in CME/Flare Initiation Brian T. Welsch Space Sciences Lab, UC-Berkeley Although CMEs and flares.
Emerging Flux Simulations Bob Stein A.Lagerfjard Å. Nordlund D. Benson D. Georgobiani 1.
Photospheric Flows and Solar Flares Brian T. Welsch 1, Yan Li 1, Peter W. Schuck 2, & George H. Fisher 1 1 Space Sciences Lab, UC-Berkeley 2 Naval Research.
Flux Emergence & the Storage of Magnetic Free Energy Brian T. Welsch Space Sciences Lab, UC-Berkeley Flares and coronal mass ejections (CMEs) are driven.
Two energy release processes for CMEs: MHD catastrophe and magnetic reconnection Yao CHEN Department of Space Science and Applied Physics Shandong University.
Global Convection Modeling (where are we heading and how does this impact HMI?) Mark Miesch HAO/NCAR, JILA/CU (Sacha Brun, Juri Toomre, Matt Browning,
Judy Karpen, Spiro Antiochos, Rick DeVore, and Mark Linton MHD Simulations of Flux Cancellation on the Sun* *Work supported by ONR and NASA.
The May 1,1998 and May 12, 1997 MURI events George H. Fisher UC Berkeley.
Flows in NOAA AR 8210: An overview of MURI progress to thru Feb.’04 Modelers prescribe fields and flows (B, v) to drive eruptions in MHD simulations MURI.
The May 1997 and May 1998 MURI events George H. Fisher UC Berkeley.