This self-contained and detailed mathematical exposition will provide graduate students and researchers with a rigorous understanding of the unique challenges of modelling the Sun's atmosphere and magnetic field, drawing upon the principles of fluid mechanics and electromagnetism to explain...
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This self-contained and detailed mathematical exposition will provide graduate students and researchers with a rigorous understanding of the unique challenges of modelling the Sun's atmosphere and magnetic field, drawing upon the principles of fluid mechanics and electromagnetism to explain observations of solar phenomena.
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