Periodicities in the Solar Wind Tenative CSI 763 Research Project Christina Henderson.
Cascades2: Quantifying Shears in the Auroral Electric Field Erik Lundberg, Paul Kintner, Cornell University Kristina Lynch, Meghan Mella, Dartmouth College.
A Tale of Two Tails: Distortions in Comet Tails and Ship “Tails”, i.e., Turbulent Ship Wakes Tail Number One: In December 2011, NASA’s Solar Dynamics Observatory.
Lecture 6.1 Lecture 6.1 ADVANCED PLASMA DIAGNOSTICTECHNIQUES Fri 23 May 2008, 1 pm LT5 Presented by Dr Ian Falconer [email protected] Room.
Mario A. Riquelme, Anatoly Spitkovsky Department of Astrophysical Sciences, Princeton University Generation of magnetic field upstream of shocks: the cosmic.
Modeling Generation and Nonlinear Evolution of Plasma Turbulence for Radiation Belt Remediation Center for Space Science & Engineering Research Virginia.
Tiled Display Walls: Spatial Audio, Glenn Bresnahan Scientific Computing and Visualization: Linux Clusters and Tiled Display Walls July 30 – August 1,
Mechanical Waves and Wave Equation A wave is a nonlocal perturbation traveling in media or vacuum. A wave carries energy from place to place without a.
Nazarenko, Warwick Dec 8 2005 Wave turbulence beyond spectra Sergey Nazarenko, Warwick, UK Collaborators: L. Biven, Y. Choi, Y. Lvov, A.C. Newell, M. Onorato,
P-24 Plasma Physics 1 Table Top Plasma Experiments LANL Critical Skills Program John Kline July 10, 2002 P-24 Plasma Physics.
Ultra-High Energy Cosmic Rays in a Structured and Magnetized Cosmic Environment Günter Sigl GReCO, Institut d’Astrophysique de Paris, CNRS .
Gyrokinetic particle-in-cell simulations of plasma microturbulence on advanced computing platforms
