VHE Gamma Ray Astronomy: a UK strategy for the next decade Paula Chadwick for the University of Durham Johannes Knapp for the University of Leeds Richard.
Energetic Neutral Atoms from Solar Flares H. S. Hudson 1, R. P. Lin 1, A. L. MacKinnon 2, J. C. Raymond 3, A. Y. Shih 1, and Wang, L. 1 1 University of.
Integrating Global MHD Models with SECCHI Observations Pete Riley, Zoran Mikic, Jon Linker, Roberto Lionello, and Slava Titov SAIC, San Diego, California.
Energetic Neutral Atoms from Solar Flares H. S. Hudson 1, S. Frewen 1, R. P. Lin 1, A. L. MacKinnon 2, J. C. Raymond 3, and A. Y. Shih 1 1 University of.
Coronal hard X-rays prior to RHESSI H. S. Hudson Space Sciences Lab, UC Berkeley.
Konstantin Belov. GZK-40, Moscow. Konstantin Belov High Resolution Fly’s Eye (HiRes) Collaboration GZK-40. INR, Moscow. May 17, 2006. measurements by fluorescence.
Davies-Cotton f/1.0 Optics. Total mirror area = 106 m 2
The High Resolution Fly’s Eye
JNM Dec. 2001 Annecy, France The High Resolution Fly’s Eye John Matthews University of Utah Department of Physics and High Energy Astrophysics Institute.
Relation between Type II Bursts and CMEs Inferred from STEREO Observations
SWG-17Pasadena, CA B A Direction Finding and Triangulation from STEREO & Wind M. J. Reiner.