On the Ekman instability at the core–mantle boundary


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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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O. Chkhetiani

Obukhov Institute of Atmospheric Physics; Space Research Institute

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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

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俄罗斯联邦, ul. B. Gruzinskaya 10, Moscow, 123995; ul. Profsoyuznaya 84/32, Moscow, 117997

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