SOLAR FLARE ENERGETIC PARTICLES Eduard Kontar School of Physics and Astronomy University of Glasgow, UK.
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,
Integrating Global MHD Models with SECCHI Observations Pete Riley, Zoran Mikic, Jon Linker, Roberto Lionello, and Slava Titov SAIC, San Diego, California.
Vincent Surges Advisors: Yingna Su Aad van Ballegooijen Observations and Magnetic Field Modeling of a flare/CME event on 2010 April 8.
How are photospheric flows related to solar flares? Brian T. Welsch 1, Yan Li 1, Peter W. Schuck 2, & George H. Fisher 1 1 SSL, UC-Berkeley 2 NASA-GSFC.
Forecasting Space Weather with Dynamic Coronal Models B.T. Welsch, W.P. Abbett, J. McTiernan, G.H. Fisher, Space Sciences Laboratory, University of California,
Mapping Free Energy in the Solar Atmosphere
Multi-Height Full Stokes Polarimetry of a B-Class Flare Tom Schad – in collaboration with – Ali Tritschler & Matt Penn CANFIELD-FEST Aug 8 – 11, 2010.
NADIR: Neutral Atmosphere Density Interdisciplinary Research -
The Sun’s Global Photospheric and Coronal Magnetic Fields Duncan H Mackay Solar Physics Group University of St. Andrews.
Manolis K. Georgoulis 1 & Thomas Wiegelmann 2
Magnetic Field Extrapolations And Current Sheets