Математическое моделирование физических процессов аномального прогрева солнечной атмосферы
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Произведена линеаризация системы уравнений НМГД и методом исключения переменных получено линейное уравнение малых колебаний магнитной трубки, расположенной в экваториальной плоскости Солнца. Вопрос устойчивости равновесных положений магнитной трубки (реализации линейных колебаний с малыми амплитудами) и неустойчивых равновесных положений (реализации нелинейных колебаний с большими амплитудами… Читать ещё >
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