岁差和北部高纬气候对安达曼海季风季节和生产力的强烈影响

IF 4 1区 地球科学 Q1 GEOGRAPHY, PHYSICAL
Rinu Fathima , Rajeev Saraswat , Sudhira R. Bhadra , Dinesh Kumar Naik , Thejasino Suokhrie
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引用次数: 0

摘要

印度季风(IM)是全球气候系统的重要组成部分,驱动着印度洋降水、生产力和环流的季节性变化。然而,尽管它对生活在南亚的10多亿人的社会经济状况产生了重大影响,但影响其时空变异性的因素仍然不确定。安达曼海是一个核心季风区,是一个独特的、样本相对较少的盆地,与全球海洋的连通性有限。为了更好地了解IM季节性和相关生产力的期间变率,我们研究了安达曼海国际海洋发现计划(IODP) 353考察队U1448站点浮游有孔虫的相对丰度。研究结果表明,印度夏季风(ISM)和印度冬季风(IWM)在间冰期和间冰期表现出较强的季节间冰期变异性。其中,最强的ISM出现在全新世早期,与较高的日照有关,而最强的IWM强度出现在Heinrich Event 1 (H1)期间。此外,高纬千年尺度北大西洋冷暖事件(如Younger Dryas (YD)、Heinrich事件(H1−10)和Bolling-Allerod事件(B/ a))对安达曼海具有强烈的影响,暖事件通常导致更强的ISM,冷事件通常导致更强的IWM。我们还报告了ISM和生产率之间的强耦合,更强的ISM与更高的生产率相关。磁化率(MS)和红蓝(R/B)反射率(R/B)具有明显的节间变率,可用于了解碳酸钙(CaCO3)和有机碳(Corg)含量的变化。间歇期CaCO3和Corg值较高,间歇期CaCO3和Corg值较低。ISM和IWM均表现出明显的周期性,分别为24和21 kyr,夏季风在岁差带与北半球最大太阳日晒处于同相,有2.4 kyr的小滞后,表明岁差在控制安达曼地区季风中起主导作用。最后一次冰期—间冰期旋回期间,太阳辐照变率受岁差调制的主要影响,同时,冰川边界条件、北半球气候和温室气体浓度等内部反馈也对太阳辐照变率产生影响。这些发现为了解影响IM变率的因素提供了重要的见解,并将有助于提高我们对气候系统复杂动态的理解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A strong influence of the precession and northern high latitudinal climate on the monsoon seasonality and productivity in the Andaman Sea
The Indian Monsoon (IM) is a vital component of the global climate system, driving seasonal changes in precipitation, productivity, and circulation in the Indian Ocean. However, despite its significance in affecting the socio-economic conditions of over a billion people living in South Asia, the factors influencing the spatio-temporal variability of IM remain uncertain. The Andaman Sea, a core monsoon region, is a unique and relatively under-sampled basin with limited connectivity to the global ocean. To better understand the stadial-interstadial variability in IM seasonality and associated productivity, we studied the relative abundance of planktic foraminifera from the International Ocean Discovery Program (IODP) Expedition 353 Site U1448 in the Andaman Sea. Our findings reveal a strong stadial-interstadial variability in the monsoon seasonality, with a stronger Indian Summer monsoon (ISM) during the interstadials and a stronger Indian Winter monsoon (IWM) during the stadials. Specifically, the strongest ISM was during the early Holocene, associated with higher insolation, while peak IWM intensity was during the Heinrich Event 1 (H1). Moreover, we observed a strong influence of the high latitudinal millennial scale North Atlantic cold and warm events, such as Younger Dryas (YD), Heinrich Event (H1−10), and Bolling-Allerod (B/A), on the Andaman Sea, with warm events typically leading to stronger ISM and cold events leading to stronger IWM. We also report a strong coupling between ISM and productivity, with stronger ISM associated with higher productivity. A distinct stadial-interstadial variability was observed in the magnetic susceptibility (MS) and Red/Blue (R/B) reflectance ratio which were used to understand the calcium carbonate (CaCO3) and organic carbon (Corg) content variability. The higher CaCO3 and Corg values were observed during the interstadials and lower values during the stadials. Both, ISM and IWM exhibited a significant periodicity of 24 and 21 kyr, respectively and the summer monsoon was in phase with maximum northern hemisphere solar insolation in the precession band with a minor lag of 2.4 kyr, suggesting the dominant role of precession in controlling the monsoon in the Andaman region. This study suggests a precession modulated insolation variability as the major factor controlling IM variability, along with which, internal feedbacks including the glacial boundary conditions, northern hemisphere climate and greenhouse gas concentration also influenced the IM during the last glacial-interglacial cycle. These findings provide crucial insights into the factors affecting IM variability and will aid in improving our understanding of the climate system's complex dynamics.
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来源期刊
Global and Planetary Change
Global and Planetary Change 地学天文-地球科学综合
CiteScore
7.40
自引率
10.30%
发文量
226
审稿时长
63 days
期刊介绍: The objective of the journal Global and Planetary Change is to provide a multi-disciplinary overview of the processes taking place in the Earth System and involved in planetary change over time. The journal focuses on records of the past and current state of the earth system, and future scenarios , and their link to global environmental change. Regional or process-oriented studies are welcome if they discuss global implications. Topics include, but are not limited to, changes in the dynamics and composition of the atmosphere, oceans and cryosphere, as well as climate change, sea level variation, observations/modelling of Earth processes from deep to (near-)surface and their coupling, global ecology, biogeography and the resilience/thresholds in ecosystems. Key criteria for the consideration of manuscripts are (a) the relevance for the global scientific community and/or (b) the wider implications for global scale problems, preferably combined with (c) having a significance beyond a single discipline. A clear focus on key processes associated with planetary scale change is strongly encouraged. Manuscripts can be submitted as either research contributions or as a review article. Every effort should be made towards the presentation of research outcomes in an understandable way for a broad readership.
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