NSF Site Visit Madison, May 1-2, 2006 Magnetic Helicity Conservation and Transport R. Kulsrud and H. Ji for participants of the Center for Magnetic Self-organization.
14 Feb 2006C4: Coronal Energy Inputs I. Mapping Free Energy in the Solar Atmosphere What can we learn from HMI & AIA? Brian Welsch, Space Sciences Lab,
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.
Coronal radiation belts? H. S. Hudson Space Sciences Lab, UC Berkeley.
Simulations of Emerging Magnetic Flux in Active Regions W. P. Abbett Space Sciences Laboratory University of California, Berkeley.
Connections Between the Magnetic Carpet and the Unbalanced Corona: New Monte Carlo Models Steven R. Cranmer & Adriaan van Ballegooijen Harvard-Smithsonian.
Rapid Changes in the Longitudinal Magnetic Field Associated with the July 23 2002 gamma -ray Flare Vasyl Yurchyshyn, Haimin Wang, Valentyna Abramenko,
Finding Photospheric Flows with I+LCT or,“Everything you always wanted to know about velocity at the photosphere, but were afraid to ask.” B. T. Welsch,
The Dynamic Evolution of Quiet Sun Magnetic Fields in the Solar Atmosphere W.P. Abbett, Space Sciences Laboratory, Univ. of California, Berkeley [email protected].
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.
Nonlinear Force-Free Field Modeling AIA/HMI Science Team Meeting Session C2 14 February 2006 Marc DeRosa on behalf of the “NLFFF Consortium” (Karel Schrijver,
How Does Free Magnetic Energy Enter the Corona? Brian Welsch, Space Sciences Lab, UC Berkeley Free magnetic energy, equivalent to departures of the coronal.
