Slide 1Mass production (Super-K) Setup of jnubeam – 3 horn 250 kA – 30-GeV proton beam of Gaussian distribution (  x,y = 0.4243 cm) – On center, parallel beam and…

Slide 1 Temporal Separation of AIA 131 Å and GOES 1-8 Å Peak Flux in Solar Flares Daniel Herman Reed College ‘15 Advisors: Dr. Kathy Reeves & Dr. Trae Winter 8/14/2014…

Slide 1 Shock Source Description: Large-Scale Hybrid Simulations Dietmar Krauss-Varban Janet Luhmann Ilan Roth Yan Li Steve Ledvina Space Sciences Laboratory, UC Berkeley…

Slide 1 Slide 2 Gamma Rays By Phil Gilley and Katie Gray Slide 3 Where do Gamma Rays Come From? Black Holes may be a source of mysterious gamma rays in our universe. The…

Slide 1 Constraints on Particle Acceleration from Interplanetary Observations R. P. Lin together with L. Wang, S. Krucker at UC Berkeley, G Mason at U. Maryland, and R. Mewaldt…

Slide 1 SCUBA Polarization results: 1998-1999 Jane Greaves, Joint Astronomy Centre, Hawaii with special thanks to: Wayne Holland, Tim Jenness, David Berry and Antonio Chrysostomou…

Slide 1 SNS Experimental FacilitiesOak Ridge X0000910/arb Neutron Instruments for Materials Research T.E. Mason Experimental Facilities Division Spallation Neutron Source…

Decay Phase of Proton and Electron SEP Events E.I. Daibog1, K. Kecskeméty2, Yu.I. Logachev1 1 Skobeltsyn Inst. of Nuclear Physics, Moscow State Univ., Russia 2 KFKI RMKI,…

Slide 1 Radio emission from CU Virginis Kitty Lo Collaborators: Justin Bray, George Hobbs, Tara Murphy, Bryan Gaensler, Don Melrose ATUC Science Meeting 24th Oct 2011 Intro…

Lecture 11: Light The Cosmic Messenger Basic Properties of Light light is a form of energy – radiative energy rate of energy output (from Sun, lightbulb, etc.) is measured…