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...
číst celé
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.
schovat popis
Recenze