On the Ekman instability at the core–mantle boundary
- Авторы: Chkhetiani O.G.1,2, Shalimov S.L.3,2
 - 
							Учреждения: 
							
- Obukhov Institute of Atmospheric Physics
 - Space Research Institute
 - Schmidt Institute of Physics of the Earth
 
 - Выпуск: Том 52, № 3 (2016)
 - Страницы: 337-343
 - Раздел: Article
 - URL: https://journals.rcsi.science/1069-3513/article/view/223653
 - DOI: https://doi.org/10.1134/S1069351316030022
 - ID: 223653
 
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Аннотация
It is shown that the instability of turbulent flows with Ekman velocity profiles in the vicinity of the core–mantle boundary leads to the formation of horizontally oriented circulating roll structures. The geophysical implications of the presence of such structures in the liquid core are explored, namely, the formation of the hot zones with enhanced conductivity and their influence on geomagnetic reversals.
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Об авторах
O. Chkhetiani
Obukhov Institute of Atmospheric Physics; Space Research Institute
							Автор, ответственный за переписку.
							Email: pmsk7@mail.ru
				                					                																			                												                	Россия, 							Pyzhevskii per. 3, Moscow, 119017; ul. Profsoyuznaya 84/32, Moscow, 117997						
S. Shalimov
Schmidt Institute of Physics of the Earth; Space Research Institute
														Email: pmsk7@mail.ru
				                					                																			                												                	Россия, 							ul. B. Gruzinskaya 10, Moscow, 123995; ul. Profsoyuznaya 84/32, Moscow, 117997						
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