SOLAR WIND TURBULENCE; WAVE DISSIPATION AT ELECTRON SCALE WAVELENGTHS S. Peter Gary Space Science Institute Boulder, CO Meeting on Solar Wind Turbulence.
Madeline Hubbard (Keene High School) Matthew Shindel (Stanwich High School) Advisors: Fathima Muzamil, Dr. Charles Farrugia, Dr. Roy Torbert Objective:
A parametric study of frequency sweep rate of chorus wave packets E. Macúšova (1), O. Santolík (1,2), P. Décrèau (3), D. A. Gurnett (4), J. S. Pickett.
VT SuperDARN Group2011 SuperDARN WorkshopJoseph Baker ([email protected]) Testing the Equipotential Magnetic Field Line Assumption Using Interhemispheric.
Studying Solar Wind Magnetic Reconnection Events using the Cluster 4-point Measurement Capability A.C. Foster 1, C.J. Owen 1, A.N. Fazakerley 1, C. Forsyth.
Transverse instability of Alfven wave : Cluster observations and heuristic explication. Olga Alexandrova LESIA, Observatoire de Paris, France. Summer school.
In-situ observations of magnetic reconnection in solar system plasma What can we export to other astrophysical environments? Alessandro Retinò, R. Nakamura.
Studying Solar Wind Magnetic Reconnection Events using Cluster. A.C. Foster 1, C.J. Owen 1, A.N. Fazakerley 1, I. J. Rae 1, C. Forsyth 1, E. Lucek 2, H.
Flexible tools for integrating observations and models Johan De Keyser Emmanuel Gamby Belgian Institute for Space Aeronomy.
Structure and Detection of Rolled-up Kelvin-Helmholtz Vortices in the Tail Flank of the Magnetosphere H. Hasegawa, M. Fujimoto, T. K. M. Nakamura, K. Takagi.
From the Sun… to Pluto… and Beyond…
Maha Ashour-Abdalla Maha Ashour-Abdalla Institute of Geophysics and Planetary Physics, and Department of Physics and Astronomy, and Department of Physics.
