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,
Determination of Geometrical and Kinematical Properties of Disk Halo CMEs Using the Elliptic Cone Model X. P. Zhao, H. Cremades, J. T. Hoeksema, Y. Liu.
Instrumental & Technical Requirements. Science objectives for helioseismology Understanding the interaction of the p-mode oscillations and the solar magnetic.
Helicity: where it comes from and what it tells us Dana Longcope, MSU Anna Malanushenko, MSU/LMSAL 8/11/10Canfield-fest Thanks: Graham Barnes, CoRA B.
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 -