B. C. Low
Abstract
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A theory of the white light transient phenomena in the solar corona is given, based on recent analytic treatments of magnetohydrodynamics.
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A theory of the white light transient phenomena in the solar corona is given, based on recent analytic treatments of magnetohydrodynamics.
Key concepts: Magnetohydrodynamics, Plasma, Physics, Corona (planetary geology), Transient (computer programming), Astrophysics, Solar physics, Computational physics