Titlebook: Advances in Space Environment Research; Volume I A. C.-L. Chian,I. H. Cairns,Y. Yan Book 2003 Springer Science+Business Media Dordrecht 200

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Magnetic Reconnection Phenomena in Interplanetary SpaceE3, Wind, etc. We discover that the observational evidence of the magnetic reconnection may be found in the various solar wind structures, such as at the boundary of magnetic cloud, near the current sheet, and small-scale turbulence structures, etc. We have developed a third order accuracy upwind co

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Recent Developments in Magnetospheric Diagnostics Using ULF Wavesd inexpensively monitored from the ground using networks of magnetometers. The most robust measurable quantity provided by magnetometer networks is signal phase and this paper emphasizes the usefulness of this parameter in a variety of ULF wave diagnostic processes ranging from equatorial to high la

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New Insights on Geomagnetic Storms from Model Simulations Using Multi-Spacecraft Dataest to ’space weather’ programs. We thus discuss the dynamical coupling of the solar wind to the Earth’s magnetosphere during several geomagnetic storms using our ring current-atmosphere interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution

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Type II Solar Radio Bursts: Theory and Space Weather Implicationsterms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances.

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Variations of the Magnetic Fields in Large Solar Flaresing how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system.

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