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 Model development for Ulysses and SOHO


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The purpose of this research is to provide scientific expertise in solar physics and in the development and use of magnetohydrodynamic (MHD) models of coronal structures for the computation of Lyman alpha scattered radiation in these structures. The specific objectives will be to run MHD models with new boundary conditions and compute resulting sca

Autor: Wu, S. T

Fuente: https://archive.org/







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