New model and field data on estimates of Antarctic Bottom Water flow through the deep Vema Channel
- 作者: Frey D.I.1, Fomin V.V.2, Diansky N.A.2,3, Morozov E.G.1, Neiman V.G.1
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隶属关系:
- Shirshov Institute of Oceanology
- Institute of Numerical Mathematics
- Zubov State Oceanographic Institute
- 期: 卷 474, 编号 1 (2017)
- 页面: 561-564
- 栏目: Oceanology
- URL: https://ogarev-online.ru/1028-334X/article/view/189910
- DOI: https://doi.org/10.1134/S1028334X17050026
- ID: 189910
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详细
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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