Observational evidences of CR acceleration at shocks chung-ming ko institute of astronomy and department of physics, national central university, taiwan.
Matt Hill Gang Li SHINE 2007 Session summary for Shock geometry & upstream and downstream phenomena 1-day session: Tuesday morning Tuesday afternoon.
Lessons for STEREO - learned from Helios Presented at the STEREO/Solar B Workshop, 17.11.2005 Rainer Schwenn, MPS Lindau [email protected] The Helios.
1 B. Klecker Max-Planck-Institut für extraterrestrische Physik, 85740 Garching, Germany Kennebunkport, MN June 9, 2010 SOHO OVERVIEW.
Seed Population for Particle Acceleration... Anywhere in the Universe Shock heating based on many factors: 1. 1. v shock : shock speed 2. 2. Bn : magnetic.
Stuart D. BaleFIELDS iCDR – Science Requirements Solar Probe Plus FIELDS Instrument CDR Science and Instrument Overview Science Requirements Stuart D.
Shock Waves in the Large Scale Structure of the Universe and Cosmic Rays Accelerated
WG3 Session#1 Monday PM :
Matt Hill Gang Li
Radio Emission from the Sun, Heliosphere, & Planets T. S. Bastian NRAO.
Electron Acceleration in Perpendicular Collisionless shocks with preexisting magnetic field fluctuations Fan Guo and Joe Giacalone With thanks to Dr. Randy.
Preparing for STEREO – revisit Helios
