从奇利卡湖沉积物中破译的全新世气候变率:对人类活动或古气旋的含义?

Barnita Banerjee , Monalisa Mallick , Mohd Amir , Abdul Hameed , Luan Ozelim , Nihar Ranjan Kar , E.V.S.S.K. Babu , K. Venkatesham , M. Venkateshwarlu , Tanveer Hassan , Vireswar Samanta , Prem Chand Kisku , Debajyoti Paul , Pankaj Kumar , Aurovinda Panda
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引用次数: 0

摘要

沿海泻湖作为陆地和海洋之间的纽带,是过去气候变化、人类活动和古气旋事件的宝贵档案。在这项研究中,我们采用多代理方法来分析沉积记录,揭示受季风和非季风因素影响的气候变化。我们的分析结合了沉积物特征,如粒度、磁化率(MS)和粘土矿物学,以推断Chilika泻湖内的高能条件。此外,我们利用Rock-Eval热解和火焰电离检测器(FID)信号的反卷积来确定存在的有机物(OM)的类型。研究结果表明,全新世早期沙尘率高、MS升高表明季风增强,与陆生有机质为主相一致。然而,在早全新世之后,随着季风强度的减弱,海洋有机质变得更加普遍,这可能与约7.7 Ka左右河口的形成有关。尽管季风在~ 4 Ka左右减弱,但MS值仍然很高,这可能是由于风成风输入增加,风成风输入输送了钛磁铁矿,导致沉积物记录中的MS升高。在~ 4 Ka之后,沉积记录表明陆相有机质大量涌入,这可能是由于形成了一个屏障吐槽,限制了海洋的影响。从这一时期开始,季风强度逐渐增加,在约1.1 Ka达到峰值,与中世纪暖期一致。在~ 1.1 Ka之后,沉积速率上升,伴随着低磁化率(MS)和高含砂量。这一阶段也显示出陆地和海洋OM的增加,以及碳酸钙₃和伊利石浓度的增加,表明高能事件的影响,可能是飓风。在~ 1.1 Ka之后,气旋活动的增强可能与此期间El Niño-Southern振荡(ENSO)强度的减弱有关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Holocene climate variability deciphered from Chilika Lagoon sediments: Implication for anthropogenic activity or paleocyclones?

Holocene climate variability deciphered from Chilika Lagoon sediments: Implication for anthropogenic activity or paleocyclones?
Coastal lagoons, acting as a link between land and sea, serve as valuable archives for past climate variations, human activities, and paleo-cyclonic events. In this study, we employ a multi-proxy approach to analyze sedimentary records and uncover climatic shifts influenced by both monsoonal and non-monsoonal factors. Our analysis incorporates sediment characteristics such as grain size, magnetic susceptibility (MS), and clay mineralogy to infer high-energy conditions within the Chilika Lagoon. Additionally, we utilize Rock-Eval pyrolysis and deconvolution of flame ionization detector (FID) signals to determine the type of organic matter (OM) present.
Findings reveal that during the Early Holocene, a high sand percentage and elevated MS indicate an intensified monsoon, coinciding with a dominance of terrestrial OM. However, as monsoonal intensity declined after the Early Holocene, marine OM became more prevalent, likely linked to the formation of an estuary around ∼7.7 Ka. Despite a weakening monsoon around ∼4 Ka, MS values remained high, possibly due to increased aeolian input, which transported titanomagnetite, contributing to elevated MS in the sediment record. After ∼4 Ka, the sedimentary record indicates a greater influx of terrestrial OM, likely due to the formation of a barrier spit that limited marine influence. From this period onward, monsoonal intensity gradually increased, peaking around ∼1.1 Ka, coinciding with the Medieval Warm Period. Following ∼1.1 Ka, sedimentation rates rose, accompanied by low magnetic susceptibility (MS) and high sand content. This phase also shows an increase in both terrestrial and marine OM, along with higher CaCO₃ and illite concentrations, suggesting the impact of high-energy events, possibly cyclones. The intensification of cyclonic activity after ∼1.1 Ka may be associated with a weakening of El Niño–Southern Oscillation (ENSO) intensity during this period.
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