1.July ‘12 – Sept’12 Guest Article:Quarterly Newsletter from SPACECover Story: Get ready for Total Solar EclipseFalcon Dragon at Australia in November 2012- First Private…

Observation of Kinetic Plasma Jets in a Coronal-Loop Simulation Experiment S. K. P. Tripathi, * P. M. Bellan, and G. S. Yun Applied Physics, California Institute of Technology,…

Slide 1 Spectral modeling and diagnostics in various astrophysical environments Jelle Kaastra SRON Slide 2 Topics Multi-temperature structure Resonance scattering in groups…

THE ORIGIN OF THE SLOW SOLAR WIND Leon Ofman Department of Physics The Catholic University of America and NASA Goddard Space Flight Center Introduction Observations by Ulysses…

Spectral modeling and diagnostics in various astrophysical environments Jelle Kaastra SRON Topics Multi-temperature structure Resonance scattering in groups of galaxies Foreground…

Hydrostatic modelling of active region EUV and X-ray emission J. Dudík 1, E. Dzifčáková 1,2, A. Kulinová 1,2, M. Karlický 2 1 – Dept. of Astronomy, Physics of the…

THE ORIGIN OF THE SLOW SOLAR WIND Leon Ofman Department of Physics The Catholic University of America and NASA Goddard Space Flight Center Introduction Observations by Ulysses…

THE INTERPLANETARY MEDIUM AND IMF The solar wind is a âhigh-bâ plasma, so the IMF is "frozen inâ; the IMF goes where the plasma goes. Intermixed with the streaming…