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Magnetism of Saturn in the origin of the visible dense rings and in their peculiarities recorded by the Cassini probe
| DOI | https://doi.org/10.1017/S1743921324002746 |
|---|---|
| Язык | Английский |
| Конференция | XXIX IAU General Assembly Место проведения: Honolulu, Hawaii, United States Даты проведения: 3-14 August, 2015 |
| Год публикации | 2024 |
| Сборник | Proceedings of the International Astronomical Union. 2024. Vol. 20, iss. S393 (Planetary Science and Exoplanets in the Era of JWST) |
| Выходные данные | P. 1-8 |
| Авторы | |
| Абстракт | Saturn’s magnetism and diamagnetism of ice can help explain the emergence of visible dense rings by transformation of the protoplanetary cloud containing ice bodies into a disk-shaped system of stable visible dense rings with extreme flatness at Saturn’s equator. It can also explain the thin structure of the rings as a whole, the sharp edges of dense rings, the existence and specific features of B-rings, and the stability of the entire dense ring system around Saturn. Additionally, it allows calculation of equilibrium separation of ice bodies, as predicted by J.C. Maxwell, with the magnetic repulsion of the ice bodies compensating for their gravitational attraction. Ключевые слова: Planetary ring divisions, planetary rings, Saturn, Solar system, astrophysical magnetism |
| Сведения о финансировании, указанные в публикации | |
| URL | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/abs/magnetism-of-saturn-in-the-origin-of-the-visible-dense-rings-and-in-their-peculiarities-recorded-by-the-cassini-probe/1ACEAEB73DC4BC907F3791E39E51CE30 |
| Дополнительные сведения |
Запись создана: 19-01-2026 13:56
Последнее изменение: 26-01-2026 15:57
Библиографическая ссылка:
Tchernyi V. V., Kapranov S. V. Magnetism of Saturn in the origin of the visible dense rings and in their peculiarities recorded by the Cassini probe // Proceedings of the International Astronomical Union. 2024. Vol. 20, iss. S393 (Planetary Science and Exoplanets in the Era of JWST). P. 1-8. https://doi.org/10.1017/S1743921324002746
[SCOPUS]
Tchernyi V. V., Kapranov S. V. Magnetism of Saturn in the origin of the visible dense rings and in their peculiarities recorded by the Cassini probe // Proceedings of the International Astronomical Union. 2024. Vol. 20, iss. S393 (Planetary Science and Exoplanets in the Era of JWST). P. 1-8. https://doi.org/10.1017/S1743921324002746
[SCOPUS]
Экспертное заключение: –
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Индексация на момент включения в базу:- Уровень БС
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Web of Science
- Статус
- Нет
- Статус
- Да
- Импакт-фактор/Квартиль(год)
- 0.121/– (2024)
- Идентификатор
- 2-s2.0-105027756428
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