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.
June 19, 2009 R. J. Strangeway – 1RBSP SWG, Redondo Beach, CA Importance of Ground Magnetometers to NASA Heliophysics Missions Several U.S. projects have.
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.
ESS 7 Lecture 13 October 29, 2008 Substorms
1 What Geomagnetism can Tell Us about the Solar Cycle? Leif Svalgaard HEPL, Stanford University Bern, 11 Nov., 2013 ISSI Workshop: The Solar Activity Cycle:
1 Recent Progress in Long-Term Variability of Solar Activity Leif Svalgaard Stanford University, California, USA Keynote Talk, SCOSTEP-13, Xi’an 西安, China.
Data Assimilation With VERB Code
