Evolution of the dipole geomagnetic field. Observations and models
- Авторы: Reshetnyak M.Y.1,2, Pavlov V.E.1,3
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Учреждения:
- Institute of Physics of the Earth
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation
- Kazan (Volga) Ul’yanov-Lenin Federal University
- Выпуск: Том 56, № 1 (2016)
- Страницы: 110-124
- Раздел: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/155525
- DOI: https://doi.org/10.1134/S0016793215060122
- ID: 155525
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Аннотация
The works on paleomagnetic observations of the dipole geomagnetic field, its variations, and reversals in the last 3.5 billion years have been reviewed. It was noted that characteristic field variations are related to the evolution of the convection processes in the liquid core due to the effect of magnetic convection and solid core growth. Works on the geochemistry and energy budget of the Earth’s core, the effect of the solid core on convection and the generation of the magnetic field, dynamo models are also considered. We consider how core growth affects the magnetic dipole generation and variations, as well as the possibility of magnetic field generation up to the appearance of the solid core. We also pay attention to the fact that not only the magnetic field but also its configuration and time variations, which are caused by the convection evolution in the core on geological timescales, are important factors for the biosphere.
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Об авторах
M. Reshetnyak
Institute of Physics of the Earth; Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation
Автор, ответственный за переписку.
Email: m.reshetnyak@gmail.com
Россия, Bol’shaya Gruzinskaya ul. 10, Moscow, 123995; Troitsk, Moscow oblast, 142190
V. Pavlov
Institute of Physics of the Earth; Kazan (Volga) Ul’yanov-Lenin Federal University
Email: m.reshetnyak@gmail.com
Россия, Bol’shaya Gruzinskaya ul. 10, Moscow, 123995; Kazan, Tatarstan
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