Numerical Simulation of the Novaya Zemlya Bora
- Authors: Efimov V.V.1, Komarovskaya O.I.1
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Affiliations:
- Marine Hydrophysical Institute, Russian Academy of Sciences
- Issue: Vol 43, No 1 (2018)
- Pages: 22-28
- Section: Article
- URL: https://journals.rcsi.science/1068-3739/article/view/230852
- DOI: https://doi.org/10.3103/S106837391801003X
- ID: 230852
Cite item
Abstract
The development of the bora in case of strong southeastern wind in the area of Novaya Zemlya in the winter-spring of 2016 is simulated using the WRF-ARW numerical atmosphere circulation model with high spatial resolution. The features of wind speed and air temperature fields are considered which define the formation of the intensive near-surface flow, the bora, over the lee western slope of the mountain range. It is demonstrated that the bora development leads to the air temperature rise over the eastern part of the Barents Sea, to the increased surface heat fluxes, and to the formation of the cloudless zone over the sea westward of Novaya Zemlya. It was found that the main reason for the bora development is the high stability of the atmospheric boundary layer over the Kara Sea. It is shown that in case of western wind the Novaya Zemlya archipelago does not exert considerable influence on the air exchange in the Kara Sea area.
About the authors
V. V. Efimov
Marine Hydrophysical Institute, Russian Academy of Sciences
Author for correspondence.
Email: vefim38@mail.ru
Russian Federation, ul. Kapitanskaya 2, Sevastopol, 299011
O. I. Komarovskaya
Marine Hydrophysical Institute, Russian Academy of Sciences
Email: vefim38@mail.ru
Russian Federation, ul. Kapitanskaya 2, Sevastopol, 299011