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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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On magnetosphere specifics of close-orbit giant exoplanetsтезисы доклада
- Авторы: Khodachenko M.L., Alexeev I., Belenkaya E., Lammer H., Zaqarashvili T., Grießmeier J.M.
- Сборник: EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France
- Тезисы
- Год издания: 2011
- Первая страница: 190
- Аннотация: A more generic view of the 'Hot Jupiter' magnetosphere structure, based on the Paraboloid Magnetospheric Model (PMM) is provided. Due to the outflow of ionized particles from the hydrodynamiccally expanding upper atmosphere, 'Hot Jupiters' should have extended magnetodisks. The magnetic field produced by magnetodisk ring currents, dominates above the contribution of intrinsic magnetic dipole of a 'Hot Jupiter' and finally determines the size and shape of the whole magnetosphere.
- Добавил в систему: Беленькая Елена Семеновна