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印度西部卡奇海岸 1008 年海啸的地质证据:对马卡兰俯冲带沿线灾害的启示。

Geological evidence for AD 1008 tsunami along the Kachchh coast, Western India: Implications for hazard along the Makran Subduction Zone.

机构信息

Active Tectonics Group, Institute of Seismological Research, Gandhinagar, India.

Department of Geology, The M. S. University of Baroda, Vadodara, India.

出版信息

Sci Rep. 2018 Nov 14;8(1):16816. doi: 10.1038/s41598-018-35193-x.

DOI:10.1038/s41598-018-35193-x
PMID:30429508
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6235955/
Abstract

The 2004 Sumatra-Andaman tsunami emphasized the catastrophic nature of such disasters and exposed our knowledge gap of the historical and palaeo events. In the aftermath of this deadly event, the thrust in palaeotsunami studies was restricted to areas in the Indian Ocean, affected by this tsunami. The northern Arabian Sea, which hosts a similar tsunamigenic source i.e. the Makran Subduction Zone (MSZ), has so far remained 'Terra-Incognita'. Here, for the first time, we report geological evidence of the 1008 AD tsunami, also mentioned as 'an enigma' in the historical reports, by identifying a >250 km long sand sheet with a landward extent of more than 250 m from the Indian coastline. Detailed sedimentology and geochemistry reveals an offshore origin of this sand sheet, from where it was eroded by a high energy wave and deposited in a supratidal environment. Optical and AMS C chronology constrains its age of deposition around 1000 AD. The shear size of the sand sheet, laterally and across the coast, along with grain size, a characteristically different provenance, are some of the major indicators, which can be useful in palaeotsunami/palaeostorm deposit distinction. Our report of the AD 1008 event from the Indian coastline, also supports the claim that the Western MSZ, albeit at longer intervals, has experienced major thrust earthquakes (M > 8) in the historical past. The proximity of this sand sheet to the shoreline does not discount the role of extremely unlikely, large storms as its causal mechanism.

摘要

2004 年苏门答腊-安达曼海啸强调了此类灾害的灾难性性质,并暴露了我们对历史和古事件的知识空白。在这场致命事件之后,古海啸研究的重点仅限于受这场海啸影响的印度洋地区。北阿拉伯海拥有类似的海啸成因源,即阿拉伯-印度俯冲带(MSZ),但迄今为止,它仍然是“未知领域”。在这里,我们首次通过识别一条从印度海岸线延伸超过 250 米、长度超过 250 公里的沙席,为 1008 年海啸提供了地质证据,该海啸在历史报告中也被称为“一个谜”。详细的沉积学和地球化学研究表明,这条沙席起源于近海,是由高能波侵蚀并在潮上带环境中沉积而成的。光学和 AMS C 年代学将其沉积年龄约束在公元 1000 年左右。沙席的剪切尺寸、侧向和沿海岸线的粒度,以及特征不同的物源,都是一些可以用于古海啸/古风暴沉积区分的主要指标。我们对印度海岸线公元 1008 年事件的报告也支持了这样一种说法,即尽管间隔时间较长,但西 MSZ 在历史上曾经历过大型推覆地震(M > 8)。这条沙席靠近海岸线,这并不能排除极其罕见的大型风暴作为其成因机制的作用。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/1d633651a404/41598_2018_35193_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/7358b9bb0c8b/41598_2018_35193_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/4edc65f06fe6/41598_2018_35193_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/169b41e0e8c6/41598_2018_35193_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/1d633651a404/41598_2018_35193_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/7358b9bb0c8b/41598_2018_35193_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/4edc65f06fe6/41598_2018_35193_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/169b41e0e8c6/41598_2018_35193_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b4c7/6235955/1d633651a404/41598_2018_35193_Fig4_HTML.jpg

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