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  • 1
    Publication Date: 2016-06-07
    Description: The two-fluid solar-wind model is extended by including the collisionless dissipation of hydromagnetic waves originating at the sun. A series of solar wind models is generated, parameterized by the total energy flux of hydromagnetic waves at the base of the model. The resulting properties of propagation and dissipating of hydromagnetic waves on this model are presented.
    Keywords: SPACE RADIATION
    Type: Solar Wind; p 248-251
    Format: application/pdf
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