Imperial College London, FETS 1 RFQ development for high power beams 1. Introduction 2. Particle dynamics in the RFQ 3. Electrodynamic design of the RF.
Homo litoreus Seashore Man Part one In a nutshell.
Sandy desert Modifications of the surface radiation budget.
V.N. Litvinenko, ElC Collaboration Meeting, Hampton University, 19-23 May, 2008 Vladimir N. Litvinenko C-AD, Brookhaven National Laboratory, Upton, NY,
Radio Jet Disruption in Cooling Cores OR, can radio jets solve the cooling core problem? OR, how do cooling cores disrupt radio jets?
ASCI/Alliances Center for Astrophysical Thermonuclear Flashes Evaporation of Clouds in Thermally Conducting, Radiative Supernova Remnants S. Orlando (1),
The Environments of Galaxies: from Kiloparsecs to Megaparsecs August 2004 Cool Cores in Galaxy Groups Ewan O’Sullivan Harvard-Smithsonian Center for Astrophysics.
Radio Jet Disruption in Cooling Cores
Crushing of interstellar gas clouds Part I - Thermal Conduction and Radiative Losses - Equations: Heat Flux: Initial conditions Cloud Mass Fraction: choose.
What is climate change? Climate change is the change in long-term weather patterns in certain regions. These changes can affect the entire Earth.
Cool Cores in Galaxy Groups
Crushing of interstellar gas clouds Part I - Thermal Conduction and Radiative Losses -