On the Ekman instability at the core–mantle boundary
- 作者: Chkhetiani O.G.1,2, Shalimov S.L.3,2
 - 
							隶属关系: 
							
- Obukhov Institute of Atmospheric Physics
 - Space Research Institute
 - Schmidt Institute of Physics of the Earth
 
 - 期: 卷 52, 编号 3 (2016)
 - 页面: 337-343
 - 栏目: Article
 - URL: https://journals.rcsi.science/1069-3513/article/view/223653
 - DOI: https://doi.org/10.1134/S1069351316030022
 - ID: 223653
 
如何引用文章
详细
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.
作者简介
O. Chkhetiani
Obukhov Institute of Atmospheric Physics; Space Research Institute
							编辑信件的主要联系方式.
							Email: pmsk7@mail.ru
				                					                																			                												                	俄罗斯联邦, 							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
				                					                																			                												                	俄罗斯联邦, 							ul. B. Gruzinskaya 10, Moscow, 123995; ul. Profsoyuznaya 84/32, Moscow, 117997						
补充文件
				
			
						
						
					
						
						
				