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Ускорение космических лучей ударными волнами

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Институт космофизических исследований и аэрономии им. Ю.Г. Шафера, СО РАН, просп. Ленина 31, Якутск, 677980, Российская Федерация

Обзор результатов теоретических исследований процессов ускорения космических лучей ударными волнами. Основное внимание уделено теории наиболее эффективного из них процесса регулярного ускорения. Изложена линейная теория этого процесса и результаты нелинейных моделей регулярного ускорения, в которых учитывается модификация структуры ударной волны ускоренными частицами. Обсуждаются возможности объяснения явлений генерации высокоэнергичных частиц, наблюдаемых в межпланетном и межзвездном пространстве, на основе регулярного механизма ускорения и ускорение ударными волнами от вспышек сверхновых, как возможный источник галактических космических лучей. Отмечаются наиболее важные нерешенные вопросы, стоящие перед теорией ускорения заряженных частиц ударными волнами. Ил. 11. Библиографических ссылок 170 (176 назв.)

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English fulltext is available at DOI: 10.1070/PU1988v031n01ABEH002534
PACS: 96.50.Fm, 98.70.Sa, 97.60.Bw, 52.65.Kj, 95.30.Qd (все)
DOI: 10.3367/UFNr.0154.198801b.0049
URL: https://ufn.ru/ru/articles/1988/1/b/
Цитата: Бережко Е Г, Крымский Г Ф "Ускорение космических лучей ударными волнами" УФН 154 49–91 (1988)
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English citation: Berezhko E G, Krymskii G F “Acceleration of cosmic rays by shock waves” Sov. Phys. Usp. 31 27–51 (1988); DOI: 10.1070/PU1988v031n01ABEH002534

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