{"title":"东赤道太平洋1000 m深度季节内洋流变率的起源及其年际调制","authors":"Yusuke Terada, Yukio Masumoto","doi":"10.1029/2025JC022754","DOIUrl":null,"url":null,"abstract":"<p>It has been shown that the intraseasonal variability in the eastern Pacific Ocean at the intermediate depth (∼1,000 m) has a large amplitude along the equator. However, our understanding of the origin and detailed characteristics of the Equatorial Deep Intra-seasonal Variability (DEIV) is still limited. In this study, we use observed data near the surface and at 1,000 m depth as well as numerical simulations to evaluate the interannual modulation of the DEIV and its relation to the upper-ocean variability. The observed meridional component of eddy kinetic energy (EKE) at 1,000 m depth depicts large intraseasonal variability in the equatorial eastern Pacific, showing a significant seasonality with its maximum in boreal winter. The meridional EKE in winter also indicates a clear interannual variation of the DEIV. The upper-layer equatorially antisymmetric intraseasonal variability, associated with the tropical instability waves, also shows significant interannual modulation with a high correlation to the meridional EKE at 1,000 m with a 3-month lag. Though temperature and velocity observations above 500 m indicate two types of oscillation with 17- and 30-day periods in the upper layer, numerical experiments reveal that during non-La Niña years, only the 30-day component can generate vertically propagating Yanai waves, which effectively form the DEIV.</p>","PeriodicalId":54340,"journal":{"name":"Journal of Geophysical Research-Oceans","volume":"130 10","pages":""},"PeriodicalIF":3.4000,"publicationDate":"2025-09-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JC022754","citationCount":"0","resultStr":"{\"title\":\"Origin of the Intraseasonal Current Variability and Its Interannual Modulation at 1,000 m Depth in the Eastern Equatorial Pacific Ocean\",\"authors\":\"Yusuke Terada, Yukio Masumoto\",\"doi\":\"10.1029/2025JC022754\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>It has been shown that the intraseasonal variability in the eastern Pacific Ocean at the intermediate depth (∼1,000 m) has a large amplitude along the equator. However, our understanding of the origin and detailed characteristics of the Equatorial Deep Intra-seasonal Variability (DEIV) is still limited. In this study, we use observed data near the surface and at 1,000 m depth as well as numerical simulations to evaluate the interannual modulation of the DEIV and its relation to the upper-ocean variability. The observed meridional component of eddy kinetic energy (EKE) at 1,000 m depth depicts large intraseasonal variability in the equatorial eastern Pacific, showing a significant seasonality with its maximum in boreal winter. The meridional EKE in winter also indicates a clear interannual variation of the DEIV. The upper-layer equatorially antisymmetric intraseasonal variability, associated with the tropical instability waves, also shows significant interannual modulation with a high correlation to the meridional EKE at 1,000 m with a 3-month lag. Though temperature and velocity observations above 500 m indicate two types of oscillation with 17- and 30-day periods in the upper layer, numerical experiments reveal that during non-La Niña years, only the 30-day component can generate vertically propagating Yanai waves, which effectively form the DEIV.</p>\",\"PeriodicalId\":54340,\"journal\":{\"name\":\"Journal of Geophysical Research-Oceans\",\"volume\":\"130 10\",\"pages\":\"\"},\"PeriodicalIF\":3.4000,\"publicationDate\":\"2025-09-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JC022754\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Geophysical Research-Oceans\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025JC022754\",\"RegionNum\":2,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"OCEANOGRAPHY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research-Oceans","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025JC022754","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"OCEANOGRAPHY","Score":null,"Total":0}
Origin of the Intraseasonal Current Variability and Its Interannual Modulation at 1,000 m Depth in the Eastern Equatorial Pacific Ocean
It has been shown that the intraseasonal variability in the eastern Pacific Ocean at the intermediate depth (∼1,000 m) has a large amplitude along the equator. However, our understanding of the origin and detailed characteristics of the Equatorial Deep Intra-seasonal Variability (DEIV) is still limited. In this study, we use observed data near the surface and at 1,000 m depth as well as numerical simulations to evaluate the interannual modulation of the DEIV and its relation to the upper-ocean variability. The observed meridional component of eddy kinetic energy (EKE) at 1,000 m depth depicts large intraseasonal variability in the equatorial eastern Pacific, showing a significant seasonality with its maximum in boreal winter. The meridional EKE in winter also indicates a clear interannual variation of the DEIV. The upper-layer equatorially antisymmetric intraseasonal variability, associated with the tropical instability waves, also shows significant interannual modulation with a high correlation to the meridional EKE at 1,000 m with a 3-month lag. Though temperature and velocity observations above 500 m indicate two types of oscillation with 17- and 30-day periods in the upper layer, numerical experiments reveal that during non-La Niña years, only the 30-day component can generate vertically propagating Yanai waves, which effectively form the DEIV.