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О происхождении магнитных полей в астрофизике (Турбулентные механизмы «динамо»)

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Содержание: Введение. Регулярные (крупномасштабные) магнитные поля. Происхождение «затравочных» магнитных полей. Симметричная задача. Генерация регулярного поля гиротропной турбулентностью. Свойства уравнения турбулентной генерации. Астрофизические примеры. Диамагнетизм турбулентной жидкости. Граничные условия. Хаотические (мелкомасштабные) магнитные поля. Трудности проблемы. Точное решение задачи в некоторой модели турбулентности. Турбулентное динамо в присутствии акустической турбулентности. Возбуждение вихрей при наличии акустической турбулентности. Есть ли все-таки турбулентное динамо хаотических полей? Нелинейная задача. Установившееся поле. Формулировка задачи. Определение величины магнитной гиротропности. Некоторые свойства магнитной гиротропности. Цитированная литература.

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English fulltext is available at DOI: 10.1070/PU1972v015n02ABEH004960
PACS: 95.85.Sz, 95.30.Qd, 96.60.Hv, 97.10.Ld (все)
DOI: 10.3367/UFNr.0106.197203b.0431
URL: https://ufn.ru/ru/articles/1972/3/b/
Цитата: Вайнштейн С И, Зельдович Я Б "О происхождении магнитных полей в астрофизике (Турбулентные механизмы "динамо")" УФН 106 431–457 (1972)
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English citation: Vainshtein S I, Zel’dovich Ya B “Origin of Magnetic Fields in Astrophysics (Turbulent ’Dynamo’ Mechanisms)” Sov. Phys. Usp. 15 159–172 (1972); DOI: 10.1070/PU1972v015n02ABEH004960

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