Jim Ulvestad Division Director, AST October 13, 2011 Division of Astronomical Sciences.
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.
Connections Between the Magnetic Carpet and the Unbalanced Corona: New Monte Carlo Models Steven R. Cranmer & Adriaan van Ballegooijen Harvard-Smithsonian.
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,
Dec 9, 2005AGU Fall 2005, San Francisco Reconnection in the Solar Corona Probing the fundamental scales Dana Longcope Montana State University Work supported.
1.B – Solar Dynamo 1.C – Global Circulation 1.D – Irradiance Sources 1.H – Far-side Imaging 1.F – Solar Subsurface Weather 1.E – Coronal Magnetic Field.
How Does Free Magnetic Energy Enter the Corona? Brian Welsch, Space Sciences Lab, UC Berkeley Free magnetic energy, equivalent to departures of the coronal.
How Does Free Magnetic Energy Enter the Corona?
Synchronic Magnetic Maps - the Inner Boundary Condition for the Heliosphere David Hathaway NASA Marshall Space Flight Center 2011 August 2 – Space Weather.
Newark, 31.03.2008Wiegelmann et al.: Coronal magnetic fields1 Solar coronal magnetic fields: Source of Space weather Thomas Wiegelmann, Julia Thalmann,
HMI Major Science Objectives NameRol e InstitutionPhase B,C,DPhase-E Philip H. ScherrerPIStanford UniversityHMI InvestigationSolar Science John G. BeckA-IStanford.
Karen Meyer University of St Andrews Scotland 1 st year PhD student (3 months in)