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The top documents tagged [closed field lines]
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closed field lines
Magnetic Reconnection: Some Answers and Open Questions Amitava Bhattacharjee Space Science Center and Center for Magnetic Self- Organization University.
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The Phase-Resolved Spectra of the Crab Pulsar Jianjun Jia Jan 3, 2006.
217 views
The flow dynamic pressure compress the magnetic field at magnetopause (MP), which while reconnected, in turn, accelerates plasma across the flow till Alfven.
213 views
Prediction of Central Axis Direction of Magnetic Clouds Xuepu Zhao and Yang Liu Stanford University The West Pacific Geophysics Meeting, Beijing, China.
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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.
213 views
Relation Between Electric Fields and Ionospheric/magnetospheric Plasma Flows at Very Low Latitudes Paul Song Center for Atmospheric Research University.
219 views
Magnetosphere-Ionosphere Coupling and Aurora at Jupiter and Saturn Emma Bunce and Stan Cowley University of Leicester, UK Image credits: John Clarke/Boston.
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International Colloquium and Workshop "Ganymede Lander: scientific goals and experiments"
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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.
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Lecture 16 Simulating from the Sun to the Mud. Space Weather Modeling Framework – 1 [Tóth et al., 2007] The SWMF allows developers to combine models without.
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The Solar Wind. The Ulysses orbit from launch through 1995.
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CDS meeting September 2005 Solar Physics at UCLan Dr Barbara Bromage Centre for Astrophysics University of Central Lancashire.
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