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首页> 外文期刊>Quaternary Science Reviews: The International Multidisciplinary Review Journal >Timing and characteristics of Late Pleistocene and Holocene wetter periods in the Eastern Desert and Sinai of Egypt, based on C-14 dating and stable isotope analysis of spring tufa deposits
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Timing and characteristics of Late Pleistocene and Holocene wetter periods in the Eastern Desert and Sinai of Egypt, based on C-14 dating and stable isotope analysis of spring tufa deposits

机译:基于C-14定年和春季石灰岩沉积物的稳定同位素分析,埃及东部沙漠和西奈半岛晚更新世和全新世湿润时期的时间和特征

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There is very little dated evidence on wet periods in the Eastern Desert and Sinai Peninsula of Egypt during the Late Pleistocene and Holocene. To obtain such information, we have studied the petrography, isotope geochemistry and AMS radiocarbon ages of mostly relict tufas deposited by springs draining perched ground water bodies in metamorphic and volcanic rocks. The tufas unconformably overly Precambrian basic igneous rocks (basalt, diabase and gabbro). As the ages of tufa carbonate are frequently older than the true ages of the deposits because of the incorporation of old, C-14-dead carbon, we have dated both the carbonate matrix and insoluble organic material of the tufas. These ages show that the tufas were largely formed during two broad time periods, the most recent from 12,058 to 6678 cal yr BP (African Humid Period), and the other from similar to 31,200-22,500 cal yr BP, with preferential growth during the coldest times of this period namely during Heinrich Events 2 and 3 (H2 and H3) and the Last Glacial Maximum (LGM). The time span between 19,000-9000 cal yr BP, including the YD and H1, appears to have been relatively more arid than the earlier LGM or H2 periods or the later Holocene. The Late Pleistocene tufas are depleted in O-18 relative to the Holocene tufas and were deposited at a lower temperature (similar to 14.0 degrees-20.8 degrees C vs. 18.4 degrees-23.4 degrees C). We believe that the Holocene tufas in the Sinai were formed by rainfall from the Mediterranean and those in the southern part of the Eastern Desert by African monsoon rainfall derived from the Red Sea-Gulf of Aden and Indian Ocean. In contrast, the moisture that fed the Late Pleistocene tufas, which are depleted in O-18 relative to Holocene deposits, and progressively depleted from north to south, was probably brought by the Westerlies from the Atlantic-Mediterranean Sea when the Westerly circulation was pushed southwards during the coldest periods of the Late Pleistocene. Periods of tufa deposition correlate with major documented paleoclimatic events in North Africa during the late Pleistocene and Holocene; such as the Nile floods, high sea level and the formation of sapropels in the Mediterranean. (C) 2015 Elsevier Ltd. All rights reserved.
机译:在晚更新世和全新世期间,埃及东部沙漠和西奈半岛的潮湿时期很少有过时的证据。为了获得这些信息,我们研究了变质和火山岩中排泄栖息地下水体的泉水沉积而成的大部分遗留的石灰石的岩石学,同位素地球化学和AMS放射性碳年龄。凝灰岩与前寒武纪基本火成岩(玄武岩,辉绿岩和辉长岩)不一致。由于掺入了旧的C-14死碳,石灰石碳酸盐的年龄通常比矿床的真实年龄大,因此我们已经对石灰石的碳酸盐基质和不溶性有机物质进行了测年。这些年龄表明,凝灰岩主要是在两个较宽的时期内形成的,最近的时期是从12058到6678 cal yr BP(非洲湿润时期),另一个时期是类似的31200-22500 cal BP,在最冷的时候优先生长这个时期的时间,即在海因里希事件2和事件3(H2和H3)以及最后一次冰河期(LGM)期间。与早期的LGM或H2时期或较晚的全新世相比,包括YD和H1在内的19,000-9000 cal BP之间的时间跨度似乎相对更干旱。晚更新世的凝灰岩相对于全新世的凝灰岩在O-18中被耗尽,并在较低的温度下沉积(类似于14.0摄氏度至20.8摄氏度与18.4摄氏度至23.4摄氏度)。我们认为,西奈的全新世的凝灰岩是由地中海的降雨形成的,而东部沙漠的南部则是由来自亚丁红海和印度洋的非洲季风降雨形成的。相比之下,当晚更新世的凝灰岩喂食的水分相对于全新世的沉积物在O-18中被耗竭,并且从北向南逐渐耗竭,这可能是由于西风推动了西大西洋人从大西洋-地中海带来的。在晚更新世最冷的时期向南。在晚更新世和全新世末期,石灰石沉积时期与北非主要的古气候事件有关。例如尼罗河洪水,高海平面以及地中海地区腐烂物的形成。 (C)2015 Elsevier Ltd.保留所有权利。

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