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Приложение задачи о вихревом слое для района течения Гольфстрим. / Сандалюк, Никита Валерьевич; Гневышев, Владимир Григорьевич; Белоненко, Татьяна Васильевна; Кочнев, А.В.

In: СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА, Vol. 18, No. 5, 2021, p. 242–251.

Research output: Contribution to journalArticlepeer-review

Harvard

Сандалюк, НВ, Гневышев, ВГ, Белоненко, ТВ & Кочнев, АВ 2021, 'Приложение задачи о вихревом слое для района течения Гольфстрим', СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА, vol. 18, no. 5, pp. 242–251. https://doi.org/10.21046/2070-7401-2021-18-5-242-251

APA

Сандалюк, Н. В., Гневышев, В. Г., Белоненко, Т. В., & Кочнев, А. В. (2021). Приложение задачи о вихревом слое для района течения Гольфстрим. СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА, 18(5), 242–251. https://doi.org/10.21046/2070-7401-2021-18-5-242-251

Vancouver

Сандалюк НВ, Гневышев ВГ, Белоненко ТВ, Кочнев АВ. Приложение задачи о вихревом слое для района течения Гольфстрим. СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА. 2021;18(5):242–251. https://doi.org/10.21046/2070-7401-2021-18-5-242-251

Author

Сандалюк, Никита Валерьевич ; Гневышев, Владимир Григорьевич ; Белоненко, Татьяна Васильевна ; Кочнев, А.В. / Приложение задачи о вихревом слое для района течения Гольфстрим. In: СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА. 2021 ; Vol. 18, No. 5. pp. 242–251.

BibTeX

@article{14637c302ef54482b3370fde157de291,
title = "Приложение задачи о вихревом слое для района течения Гольфстрим",
abstract = "In this paper, the main statements of the problem of a non-zonal vortex layer on the β-plane in the Miles - Ribner formulation are applied to observations in the real ocean. Earlier, we showed that when waves interact with a non-zonal flow, a new class of solutions appears, which is absent in the case of a zonal flow. This new class of solutions can be interpreted as pure radiation of Rossby waves by a nonzonal flow. The analysis of the space-time diagrams in the region under consideration confirms the previously obtained theoretical conclusions of the problem of the interaction of planetary waves with a non-zonal flow on the β-plane in the Miles - Ribner formulation. Incident, reflected and refracted waves are distinguished. It is shown that Rossby waves propagating from east to west at a speed of 7.6 cm/s are transformed into refracted and reflected waves when interacting with the current. The refracted waves propagate against the current, to the southwest, at a speed of 4.6 cm/s. The reflected waves propagate to the southeast, perpendicular to the current, at a speed of 7.8 cm/s. The speed of reflected waves exceeds the speed of incident waves, which confirms the conclusions about the existence of mechanisms for amplifying planetary waves when they interact with a non-zonal flow.",
keywords = "Altimetry, Flow, Gulf Stream, Incident, Reflected, Refracted wave, Rossby waves, Vortex layer, WKB approximation, Altimetry, Flow, Gulf Stream, Incident, Reflected, Refracted wave, Rossby waves, Vortex layer, WKB approximation",
author = "Сандалюк, {Никита Валерьевич} and Гневышев, {Владимир Григорьевич} and Белоненко, {Татьяна Васильевна} and А.В. Кочнев",
year = "2021",
doi = "10.21046/2070-7401-2021-18-5-242-251",
language = "русский",
volume = "18",
pages = "242–251",
journal = "СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА",
issn = "2070-7401",
publisher = "Институт космических исследований Российской академии наук",
number = "5",

}

RIS

TY - JOUR

T1 - Приложение задачи о вихревом слое для района течения Гольфстрим

AU - Сандалюк, Никита Валерьевич

AU - Гневышев, Владимир Григорьевич

AU - Белоненко, Татьяна Васильевна

AU - Кочнев, А.В.

PY - 2021

Y1 - 2021

N2 - In this paper, the main statements of the problem of a non-zonal vortex layer on the β-plane in the Miles - Ribner formulation are applied to observations in the real ocean. Earlier, we showed that when waves interact with a non-zonal flow, a new class of solutions appears, which is absent in the case of a zonal flow. This new class of solutions can be interpreted as pure radiation of Rossby waves by a nonzonal flow. The analysis of the space-time diagrams in the region under consideration confirms the previously obtained theoretical conclusions of the problem of the interaction of planetary waves with a non-zonal flow on the β-plane in the Miles - Ribner formulation. Incident, reflected and refracted waves are distinguished. It is shown that Rossby waves propagating from east to west at a speed of 7.6 cm/s are transformed into refracted and reflected waves when interacting with the current. The refracted waves propagate against the current, to the southwest, at a speed of 4.6 cm/s. The reflected waves propagate to the southeast, perpendicular to the current, at a speed of 7.8 cm/s. The speed of reflected waves exceeds the speed of incident waves, which confirms the conclusions about the existence of mechanisms for amplifying planetary waves when they interact with a non-zonal flow.

AB - In this paper, the main statements of the problem of a non-zonal vortex layer on the β-plane in the Miles - Ribner formulation are applied to observations in the real ocean. Earlier, we showed that when waves interact with a non-zonal flow, a new class of solutions appears, which is absent in the case of a zonal flow. This new class of solutions can be interpreted as pure radiation of Rossby waves by a nonzonal flow. The analysis of the space-time diagrams in the region under consideration confirms the previously obtained theoretical conclusions of the problem of the interaction of planetary waves with a non-zonal flow on the β-plane in the Miles - Ribner formulation. Incident, reflected and refracted waves are distinguished. It is shown that Rossby waves propagating from east to west at a speed of 7.6 cm/s are transformed into refracted and reflected waves when interacting with the current. The refracted waves propagate against the current, to the southwest, at a speed of 4.6 cm/s. The reflected waves propagate to the southeast, perpendicular to the current, at a speed of 7.8 cm/s. The speed of reflected waves exceeds the speed of incident waves, which confirms the conclusions about the existence of mechanisms for amplifying planetary waves when they interact with a non-zonal flow.

KW - Altimetry

KW - Flow

KW - Gulf Stream

KW - Incident

KW - Reflected

KW - Refracted wave

KW - Rossby waves

KW - Vortex layer

KW - WKB approximation

KW - Altimetry

KW - Flow

KW - Gulf Stream

KW - Incident

KW - Reflected

KW - Refracted wave

KW - Rossby waves

KW - Vortex layer

KW - WKB approximation

UR - http://www.scopus.com/inward/record.url?scp=85120375394&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/c25fff24-be62-3ead-a590-6962732b386b/

U2 - 10.21046/2070-7401-2021-18-5-242-251

DO - 10.21046/2070-7401-2021-18-5-242-251

M3 - статья

VL - 18

SP - 242

EP - 251

JO - СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА

JF - СОВРЕМЕННЫЕ ПРОБЛЕМЫ ДИСТАНЦИОННОГО ЗОНДИРОВАНИЯ ЗЕМЛИ ИЗ КОСМОСА

SN - 2070-7401

IS - 5

ER -

ID: 88341676