New model and field data on estimates of Antarctic Bottom Water flow through the deep Vema Channel


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We used a numerical model of the ocean circulation with a high spatial resolution to obtain estimates of the kinematic characteristics of Antarctic Bottom Water flow through the abyssal Vema Channel in the southwestern part of the Atlantic Ocean. The results of simulations correspond to the data of direct velocity measurements made at several locations in the channel. The high horizontal and vertical resolution of the model in the bottom layer allowed us to study in detail the hydrodynamics of this flow over its entire length.

作者简介

D. Frey

Shirshov Institute of Oceanology

Email: lihar89@mail.ru
俄罗斯联邦, Moscow, 117218

V. Fomin

Institute of Numerical Mathematics

编辑信件的主要联系方式.
Email: lihar89@mail.ru
俄罗斯联邦, Moscow, 119991

N. Diansky

Institute of Numerical Mathematics; Zubov State Oceanographic Institute

Email: lihar89@mail.ru
俄罗斯联邦, Moscow, 119991; Moscow, 119034

E. Morozov

Shirshov Institute of Oceanology

Email: lihar89@mail.ru
俄罗斯联邦, Moscow, 117218

V. Neiman

Shirshov Institute of Oceanology

Email: lihar89@mail.ru
俄罗斯联邦, Moscow, 117218

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