VSO Integration with netDRMS Joseph A. Hourclé and the VSO Team HMI : 2009 Sept 08.
Empirical Forecasting of CMEs from a Free-Energy Proxy: Performance and Extension to HMI David Falconer, Ron Moore, Abdulnasser F. Barghouty, & Igor Khazanov.
The Solar Group is ~30 people working to better understand the Sun and the sources of its variability. There are several projects including one on the.
Structure of a Transition Region Explosive Event
19 Oct 2005SPW41 Penumbral MMFs S Jaeggli (UHawaii) C Henney (NSO) S Luszcz (Cornell) S Walton (CSUN/SFO)
Valentina Abramenko Big Bear Solar Observatory of NJIT
Detection and Analysis of Magnetic Fragments within Solar Active Regions
Solar Physics & upper-Atmosphere Research Group Robert Erdélyi University of SheffieldPPARC ASSSP 2006 31 Aug – 4 Sep.
Comparing solar internal rotation results from MDI and GONG R. Howe 1, J. Christensen-Dalsgaard 2, F. Hill 1, R. W. Komm 1, J. Schou 3, M. J. Thompson.
Fraser Watson, University of Glasgow Lyndsay Fletcher, University of Glasgow Stephen Marshall, University of Strathclyde SIPwork V, Wed September 15th.
Time-Distance Helioseismology from HMI
Comparison of Near-Surface Flows Assessed by Ring-Diagram and F-Mode Time-Distance Analyses