An introduction to the physics of the interstellar medium I. Overview II. Thermal processes in the ISM III. Hydrodynamics in the ISM IV. Gravity in the.
CHAP Meeting 4 October 2007 CISL Update Operations and Services CISL HPC Advisory Panel Meeting 4 October 2007 Tom Bettge Director of Operations and Services.
Paradigm Change in Fusion Science and University Research Centers in Korea Hyeon K. Park Pohang University of Science and Technology (POSTECH) at 2008.
Capabilities of UV Coronagraphic Spectroscopy for Studying the Source Regions of SEPs & the Solar Wind John Kohl, Steven Cranmer, Larry Gardner, Jun Lin,
The COMPLETE Survey of Star-Forming Regions: Nature vs. Nurture Alyssa A. Goodman Harvard-Smithsonian Center for Astrophysics cfa-agoodman.
WIYN Image: T.A. Rector, B. Wolpa and G. Jacoby (NOAO/AURA/NSF) and Hubble Heritage Team (STScI/AURA/NASA) Stars Forming in a Dynamic Interstellar Medium.
Spectroscopic Diagnostics of Solar Wind, CME, and SEP Source Regions Imaging Workshop, NSSTC, Huntsville, AL, 9-10 November 2004 Spectroscopic Diagnostics.
Review of MHD simulations of accretion disks MHD simulations of disk winds & protostellar jets Describe new Godunov+CT MHD Code Tests Application to MRI.
Interplanetary Scintillations and the Acceleration of the Solar Wind Steven R. Spangler …. University of Iowa.
Stellar Wind Theory Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics with A. van Ballegooijen, S. Saar, A. Dupree, N. Brickhouse, et al.
Three-dimensional MHD simulations of emerging flux and associated magnetic reconnection Hiroaki Isobe (DAMTP, Cambridge / Tokyo) Takehiro Miyagoshi, Kazunari.
LM-MHD Simulation Development and Recent Results Presented by Sergey Smolentsev (UCLA) with contribution from: R. Munipalli, P. Huang (HyPerComp) M. Abdou,