New model and field data on estimates of Antarctic Bottom Water flow through the deep Vema Channel
- Authors: Frey D.I.1, Fomin V.V.2, Diansky N.A.2,3, Morozov E.G.1, Neiman V.G.1
-
Affiliations:
- Shirshov Institute of Oceanology
- Institute of Numerical Mathematics
- Zubov State Oceanographic Institute
- Issue: Vol 474, No 1 (2017)
- Pages: 561-564
- Section: Oceanology
- URL: https://ogarev-online.ru/1028-334X/article/view/189910
- DOI: https://doi.org/10.1134/S1028334X17050026
- ID: 189910
Cite item
Abstract
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.
About the authors
D. I. Frey
Shirshov Institute of Oceanology
Email: lihar89@mail.ru
Russian Federation, Moscow, 117218
V. V. Fomin
Institute of Numerical Mathematics
Author for correspondence.
Email: lihar89@mail.ru
Russian Federation, Moscow, 119991
N. A. Diansky
Institute of Numerical Mathematics; Zubov State Oceanographic Institute
Email: lihar89@mail.ru
Russian Federation, Moscow, 119991; Moscow, 119034
E. G. Morozov
Shirshov Institute of Oceanology
Email: lihar89@mail.ru
Russian Federation, Moscow, 117218
V. G. Neiman
Shirshov Institute of Oceanology
Email: lihar89@mail.ru
Russian Federation, Moscow, 117218
Supplementary files
