Cluster Reveals Properties of Cold Plasma Flow May 15, 2009 Erik Engwall.
THE AURORAL EMISSIONS AND THE ELECTRON PRECIPITATION UNDER DIFFERENT GEOMAGNETIC CONDITIONS DURING RECURRENT SOLAR WIND STREAM Guineva V. 1, Despirak I.
Anti-Parallel Merging and Component Reconnection: Role in Magnetospheric Dynamics M.M Kuznetsova, M. Hesse, L. Rastaetter NASA/GSFC T. I. Gombosi University.
ESS 200C Lecture 12 Planetary Magnetospheres. We have studied the Earth’s magnetosphere in great detail for over 40 years and think we have developed.
CISM Advisory Council Meeting 4 March 2003 Magnetospheric Modeling Mary K. Hudson and the CISM Magnetospheric Modeling Team.
ENLIL 3D-MHD Modeling Support of Heliospheric Missions European Space Weather Week, Liege, Belgium, 17-21 November 2014 Dusan Odstrcil (GMU & NASA/GSFC)
Figure 1: show a causal chain for how Joule heating occurs in the earth’s ionosphere Figure 5: Is of the same format as figure four but the left panels.
June 19, 2009 R. J. Strangeway – 1RBSP SWG, Redondo Beach, CA Importance of Ground Magnetometers to NASA Heliophysics Missions Several U.S. projects have.
Combined Effects of Concurrent Pc5 and Chorus Waves on Relativistic Electron Dynamics Christos Katsavrias 1,2, Ioannis A. Daglis 2,1, Wen Li 3, Stavros.
Intermittency beyond the ecliptic plane Anna Wawrzaszek, Marius Echim, Wiesław M. Macek, Roberto Bruno Mamaia, 6-13 September 2015 (1) Space Research Centre.
Determining the Location of Open Magnetic Field Areas in Active Regions and their Potential as Sources of the Slow Solar Wind J. L. Culhane 1, S.J. Edwards.
Solar cycle dependence of EMIC wave frequencies Marc Lessard, Carol Weaver, Erik LindgrenMark Engebretson University of New HampshireAugsburg College Introduction.