Emergence of an equatorial mode of climate variability in the Indian Ocean

被引:24
|
作者
DiNezio, Pedro N. [1 ]
Puy, Martin [1 ]
Thirumalai, Kaustubh [2 ]
Jin, Fei-Fei [3 ]
Tierney, Jessica E. [2 ]
机构
[1] Univ Texas Austin, Jackson Sch Geosci, Inst Geophys, JJ Pickle Res Campus,Bldg 196,10100 Burnet Rd, Austin, TX 78758 USA
[2] Univ Arizona, Dept Geosci, 1040 E 4th St, Tucson, AZ 85721 USA
[3] Univ Hawaii Manoa, Dept Atmospher Sci, 2525 Correa Rd, Honolulu, HI 96822 USA
来源
SCIENCE ADVANCES | 2020年 / 6卷 / 19期
关键词
SEA-SURFACE TEMPERATURE; PACIFIC COLD-TONGUE; INDO-PACIFIC; DIPOLE; DYNAMICS; CMIP5; ENSO; UPGRADES; PATTERN; EVENTS;
D O I
10.1126/sciadv.aay7684
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Presently, the Indian Ocean (IO) resides in a climate state that prevents strong year-to-year climate variations. This may change under greenhouse warming, but the mechanisms remain uncertain, thus limiting our ability to predict future changes in climate extremes. Using climate model simulations, we uncover the emergence of a mode of climate variability capable of generating unprecedented sea surface temperature and rainfall fluctuations across the IO. This mode, which is inhibited under present-day conditions, becomes active in climate states with a shallow thermocline and vigorous upwelling, consistent with the predictions of continued greenhouse warming. These predictions are supported by modeling and proxy evidence of an active mode during glacial intervals that favored such a state. Because of its impact on hydrological variability, the emergence of such a mode would become a first-order source of climate-related risks for the densely populated IO rim.
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收藏
页数:9
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