Antenna.systems..electronic.warfare.applications
Magnetic Reconnection: Some Answers and Open Questions Amitava Bhattacharjee Space Science Center and Center for Magnetic Self- Organization University.
The Phase-Resolved Spectra of the Crab Pulsar Jianjun Jia Jan 3, 2006.
The flow dynamic pressure compress the magnetic field at magnetopause (MP), which while reconnected, in turn, accelerates plasma across the flow till Alfven.
Energetic Neutral Atoms from Solar Flares H. S. Hudson 1, R. P. Lin 1, A. L. MacKinnon 2, J. C. Raymond 3, A. Y. Shih 1, and Wang, L. 1 1 University of.
Prediction of Central Axis Direction of Magnetic Clouds Xuepu Zhao and Yang Liu Stanford University The West Pacific Geophysics Meeting, Beijing, China.
Energetic Neutral Atoms from Solar Flares H. S. Hudson 1, S. Frewen 1, R. P. Lin 1, A. L. MacKinnon 2, J. C. Raymond 3, and A. Y. Shih 1 1 University of.
Relation Between Electric Fields and Ionospheric/magnetospheric Plasma Flows at Very Low Latitudes Paul Song Center for Atmospheric Research University.
Magnetosphere-Ionosphere Coupling and Aurora at Jupiter and Saturn Emma Bunce and Stan Cowley University of Leicester, UK Image credits: John Clarke/Boston.
International Colloquium and Workshop "Ganymede Lander: scientific goals and experiments"
1. MHD-Stability of magnetotail equilibria 2. Remarks
X-ray effects on protoplanetary disks Eric Feigelson (Penn State University) 1.Review of X-ray flaring from YSOs 2.Evidence for X-ray irradiation of disks.