Variability of the Subantarctic Mode Water Volume in the South Indian Ocean During 2004-2018

被引:25
作者
Hong, Yu [1 ,2 ]
Du, Yan [1 ,2 ,3 ]
Qu, Tangdong [4 ]
Zhang, Ying [1 ,2 ]
Cai, Wenju [5 ,6 ,7 ]
机构
[1] Chinese Acad Sci, South China Sea Inst Oceanol, State Key Lab Trop Oceanog, Guangzhou, Peoples R China
[2] Southern Marine Sci & Engn Guangdong Lab, Guangzhou, Peoples R China
[3] Univ Chinese Acad Sci, Beijing, Peoples R China
[4] Univ Calif Los Angeles, Joint Inst Reg Earth Syst Sci & Engn, Los Angeles, CA USA
[5] CSIRO Oceans & Atmosphere, Ctr Southern Hemisphere Oceans Res CSHOR, Hobart, Tas, Australia
[6] Ocean Univ China, Inst Adv Ocean Studies, Key Lab Phys Oceanog, Qingdao, Peoples R China
[7] Qingdao Natl Lab Marine Sci & Technol, Qingdao, Peoples R China
基金
中国国家自然科学基金; 美国国家科学基金会;
关键词
subantarctic mode water; South Indian Ocean; INTERMEDIATE WATER; DECADAL CHANGES; CIRCULATION; IMPACT; MASSES; SUBDUCTION; DRIVEN; CO2;
D O I
10.1029/2020GL087830
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
An analysis of Argo data reveals that the subantarctic mode water (SAMW) in the South Indian Ocean (SIO), characterized by a vertical potential vorticity (PV) minimum, decreases by 10% in volume from 2004 to 2018. Most of this decrease occurs at the 26.8-26.9 kgm(-3) density range which forms southwest of Australia, while a slight volume increase occurs at 26.6-26.8 kg m(-3). Further analysis indicates that the weakening of the Mascarene High and westerly winds in the SIO reduces the evaporation-precipitation, surface heat flux, and Ekman pumping and shoals the mixed layer southwest of Australia, which leads to a volume decrease at 26.8-26.9 kg m(-3) in approximately 3 years. West of 90 degrees E, the parameters exhibit the opposite change, leading to a volume increase at 26.6-26.8 kg m(-3). This result suggests that surface winds play an important role in the variability of the SIO SAMW volume during the Argo period.
引用
收藏
页数:9
相关论文
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