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Decadal variability of tropical Indian Ocean sea surface temperature and its impact on the Indian summer monsoon

机译:热带印度洋海景温度及其对印度夏季季风影响的二等迁易率

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摘要

Decadal variability of climate over the Pacific and Atlantic Ocean is well studied. However, the decadal climate variability over the Indian Ocean and its possible impact on the summer monsoon received relatively less attention. The present study aims to explore the decadal variability of the Tropical Indian Ocean (TIO) sea surface temperature (SST) and its associations with the Indian summer monsoon rainfall (ISMR) variability. More than a hundred years of observed monthly SST data from Extended Reconstructed sea surface temperature and rainfall data from India Meteorological Department are used for the analysis. In addition to these, century reanalysis fields of winds, moisture, vertical velocity, tropospheric temperature, and sea level pressure are used for diagnosing different processes. Time series and wavelet analysis confirmed the presence of decadal variability (similar to 9 to 30 years) in the TIO SST. The decadal variance of TIO SST is maximum in the eastern equatorial Indian Ocean, followed by the north Arabian Sea. Decadal EOF of TIO SST shows a dominant basin-wide mode explaining about 50% of total variance and has robust decadal variability during 1940 to 1952; wavelet analysis supported this robust signal statistically. Similar analysis for the ISMR reveals that the decadal variance of rainfall has significant strength over monsoon core zone and Western Ghats. The EOF analysis further confirms this spatial pattern of rainfall decadal variability over India. Correlation between of decadal TIO SST and over monsoon core zone (MCZ) rainfall is significant with 2 years lag. To understand how the decadal variability of TIO SST influences the ISMR, monsoon features during strong warm and cold phase are studied. During the warm phase, MCZ and Western Ghats receive more rain than normal and vice versa for cold phase. Which is consistent with strong southwesterly winds, strong pressure gradient, and strong convergence over the MCZ for the warm phase. Also, during the warm phase, positive anomaly of mid-troposphere temperature, vertical velocity, and moist static energy are found to be associated with excess convective activity. Apart from this, larger scale zonal (Walker) and meridional (Hadley) circulation fields are also in phase with the TIO SST and rainfall variability. Our study advocates that decadal variability in TIO SST influences the monsoon dynamics and moist thermodynamics leading to near in-phase changes in the rainfall over the MCZ and Western Ghats region.
机译:在太平洋和大西洋上的气候变异性很好。然而,印度洋上的截止额外气候变化及其对夏季季风的可能影响相对不那么关注。本研究旨在探讨热带印度洋(TIO)海面温度(SST)及其与印度夏季季风降雨(ISMR)变异性的协会的十二次变化。从延长重建的海面温度和印度气象部门的降雨数据中观察到的每月SST数据超过一百年的SST数据用于分析。除此之外,还用于诊断不同工艺的潮流,水分,垂直速度,对流层温度和海平面压力。时间序列和小波分析证实了TIO SST中的二等变异性(类似于9至30岁)的存在。 TiO SST的Decadal差异在东部赤道印度洋最多,其次是北阿拉伯海。 TiO SST的Decadal Eof显示了一个主导的盆地模式,解释了总方差约50%,在1940年至1952年期间具有强大的二道变异性;小波分析在统计上支持这种强大信号。类似的ISMR的分析表明,降雨的二等差异在季风核心区和西止浦具有重大优势。 EOF分析进一步证实了这种在印度的降雨过度变异性的空间模式。二数滴度与季风核心区(MCZ)降雨与2年的滞后性有关。为了了解TiO SST的二等变异性如何影响ISMR,在强烈的温暖和冷阶段期间的季风特征。在温暖的阶段,MCZ和西部戈​​斯比正常的雨从正常接受,反之亦然。这与强烈的西南风,强大的压力梯度强,对温度的强烈收敛性强烈符合。此外,在温度期间,发现中层温度,垂直速度和潮湿的静态能量的正异常与过量的对流活动相关。除此之外,大规模的Zonal(Walker)和子午线(Hadley)循环场也与TiO SST和降雨变异相同。我们的研究倡导TiO SST的二数变异性影响季风动力学和潮湿的热力学,导致MCZ和西球山脉地区降雨区的接近相变。

著录项

  • 来源
    《Theoretical and applied climatology 》 |2020年第2期| 551-566| 共16页
  • 作者单位

    Indian Inst Trop Meteorol Pune 411008 Maharashtra India|Savitribai Phule Pune Univ Dept Atmospher & Space Sci Pune Maharashtra India;

    Indian Inst Trop Meteorol Pune 411008 Maharashtra India|Savitribai Phule Pune Univ Dept Atmospher & Space Sci Pune Maharashtra India;

    Indian Inst Trop Meteorol Pune 411008 Maharashtra India;

    Indian Inst Trop Meteorol Pune 411008 Maharashtra India;

    Indian Inst Trop Meteorol Pune 411008 Maharashtra India;

    Indian Inst Trop Meteorol Pune 411008 Maharashtra India;

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