Seasonal Variations in the Barrier Layer and Its Formation Mechanism in the Northern Indian Ocean

IF 3.3 2区 地球科学 Q1 OCEANOGRAPHY Journal of Geophysical Research-Oceans Pub Date : 2024-09-21 DOI:10.1029/2024JC020877
Ying Liu, You-Fang Yan
{"title":"Seasonal Variations in the Barrier Layer and Its Formation Mechanism in the Northern Indian Ocean","authors":"Ying Liu,&nbsp;You-Fang Yan","doi":"10.1029/2024JC020877","DOIUrl":null,"url":null,"abstract":"<p>Understanding the impact of the ocean barrier layer (BL) on regional ocean dynamics requires the knowledge of BL variability and the factors influencing it. Herein, using SODA reanalysis data sets, we systematically investigate the seasonal variations and formation mechanisms of BLs in the North Indian Ocean (NIO). Our results show that BLs are mainly found in the southeastern Arabian Sea (SEAS), Bay of Bengal (BoB), and the Eastern Equatorial Indian Ocean (EEIO), with the thickest BLs occurring in SEAS and BoB in January, and in EEIO in November. Seasonal BL variability is primarily driven by isothermal layer (IL) modulation. Further budget analysis reveals that the factors affecting seasonality of BL variability through modulating IL differ across the three regions. In the SEAS, BL variability is primarily modulated by ocean vertical processes, notably oceanic planetary waves and Ekman pumping. In the BoB, vertical dynamics, including Ekman pumping and oceanic planetary waves, are the primary determinant of BL variability, while horizontal advection affects the spatial extent of BL. In the EEIO, equatorial upwelling and oceanic planetary waves significantly affect BL variability. These results contribute to a better understanding of regional ocean dynamics and may improve the accuracy of ocean state estimates and representation of BL processes using ocean model simulations.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"129 9","pages":""},"PeriodicalIF":3.3000,"publicationDate":"2024-09-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research-Oceans","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JC020877","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"OCEANOGRAPHY","Score":null,"Total":0}
引用次数: 0

Abstract

Understanding the impact of the ocean barrier layer (BL) on regional ocean dynamics requires the knowledge of BL variability and the factors influencing it. Herein, using SODA reanalysis data sets, we systematically investigate the seasonal variations and formation mechanisms of BLs in the North Indian Ocean (NIO). Our results show that BLs are mainly found in the southeastern Arabian Sea (SEAS), Bay of Bengal (BoB), and the Eastern Equatorial Indian Ocean (EEIO), with the thickest BLs occurring in SEAS and BoB in January, and in EEIO in November. Seasonal BL variability is primarily driven by isothermal layer (IL) modulation. Further budget analysis reveals that the factors affecting seasonality of BL variability through modulating IL differ across the three regions. In the SEAS, BL variability is primarily modulated by ocean vertical processes, notably oceanic planetary waves and Ekman pumping. In the BoB, vertical dynamics, including Ekman pumping and oceanic planetary waves, are the primary determinant of BL variability, while horizontal advection affects the spatial extent of BL. In the EEIO, equatorial upwelling and oceanic planetary waves significantly affect BL variability. These results contribute to a better understanding of regional ocean dynamics and may improve the accuracy of ocean state estimates and representation of BL processes using ocean model simulations.

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
北印度洋阻挡层的季节变化及其形成机制
要了解海洋阻挡层(BL)对区域海洋动力学的影响,就必须了解海洋阻挡层的变化及其影响因素。在此,我们利用 SODA 再分析数据集,系统地研究了北印度洋(NIO)阻挡层的季节变化和形成机制。结果表明,BLs 主要分布在阿拉伯海东南部(SEAS)、孟加拉湾(BoB)和东赤道印度洋(EEIO),其中最厚的 BLs 出现在 1 月份的阿拉伯海东南部和孟加拉湾,以及 11 月份的东赤道印度洋。BL的季节性变化主要受等温层(IL)调制的驱动。进一步的预算分析表明,通过等温层调制影响 BL 变率季节性的因素在三个地区有所不同。在东南大西洋,BL 变率主要受海洋垂直过程的调节,特别是海洋行星波和 Ekman 泵。在 BoB,垂直动力学,包括 Ekman 泵和大洋行星波,是 BL 变化的主要决定因素,而水平平流则影响 BL 的空间范围。在EEIO,赤道上升流和大洋行星波对BL的变化有显著影响。这些结果有助于更好地了解区域海洋动力学,并可提高海洋状态估计的准确性,以及利用海洋模式模拟对BL过程的表述。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
Journal of Geophysical Research-Oceans
Journal of Geophysical Research-Oceans Earth and Planetary Sciences-Oceanography
CiteScore
7.00
自引率
13.90%
发文量
429
期刊最新文献
Two Types of Intraseasonal Variability With a Vertical Difference in the Currents East of Luzon Island and Their Sources An Improved Bio-Physical Parameterization for Ocean Radiant Heating in Conditions of Near-Surface Stratification Beach and Backward Bragg Sea-Swell Wave Reflection Across Rocky and Sandy Shores The Influence of Surface Fluxes on Export of Southern Ocean Intermediate and Mode Water in Coupled Climate Models Extremes and Short-Term Fluctuations in Coastal Ocean Acidification and Hypoxia
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1