Сильные возмущения солнечного ветра и динамика магнитосферы под их воздействием
Диссертация
Впервые теорию протяженной солнечной короны выдвинул Чепмен, который рассматривал солнечную корону как статическую атмосферу, перенос энергии в которой осуществляется только за счет теплопроводности. В своей пионерской работе Паркер, анализируя условия равновесия вещества короны, показал, что модель статической короны Чепмена дает слишком высокие значения давления на бесконечности по сравнению… Читать ещё >
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