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Plasma Processes on the Sun and in the Solar System (No.100425312)


Funded by

Chinese Academy of Sciences

Start Date: 2005-01-01       End Date: 2007-01-01

In this project, on the basis of magnetohydrodynamic two-fluid model generation and propagation problems of different waves (dispersion Alfven waves, Rossby-Alvfen waves, magnetohydrodynamic waves , etc.) are investigated. The interaction of the induction electric current and spatially inhomogeneous magnetic field is taken into account. Doing so we substantially enrich the class of possible low-frequency waves in the solar atmosphere and the Sun-Earth space, resolve uncertainties, fill in gaps in the present understanding, and improve the existing physical and mathematical models. Investigation is performed by both analytical and numerical methods. To form relevant physical models ground based and satellite data is used.

Project members: