J-M. Martins, M. Meybecks , V.N. Nijampurkar , B.L.K. Somayajulu
{"title":"Pavin湖中的210Pb, 226Ra和32Si(法国中部地块)","authors":"J-M. Martins, M. Meybecks , V.N. Nijampurkar , B.L.K. Somayajulu","doi":"10.1016/0168-9622(92)90010-8","DOIUrl":null,"url":null,"abstract":"<div><p>Measurements of cosmogenic <sup>32</sup>Si and the U-decay series' nuclides <sup>210</sup>Ph and <sup>226</sup>Ra in waters and sediments of lake Pavin are reported. Both <sup>210</sup>Pb and <sup>226</sup>Ra are enriched in the anoxic deep waters compared to the oxic surface waters, respectively by a factor of 4 and 10, whereas <sup>32</sup>Si is depleted by a factor of ∼ 2. Redox conditions in the lake appear to have no marked effect on the <sup>32</sup>Si. Using a steady-state box model it is shown that the deep-water <sup>32</sup>Si concentration is controlled by the underground lacustrine springs. The residence times of <sup>210</sup>Pb, <sup>32</sup>Si and <sup>226</sup>Ra are ∼ 1, ∼ 10 and ∼ 80 a, respectively. In the case of <sup>32</sup>Si where more data are available, the assessed inventory data from the overhead atmospheric fallout and that measured in the sediments agree very well as expected. The <sup>210</sup>Pb, and <sup>32</sup>Si-based deposition rates during the past ∼ 100 a ranged from 0.8 to 1.9 mm a<sup>−1</sup>, earlier these were a factor of ∼ 3–5 faster. The geochemistry of <sup>32</sup>Si and <sup>210</sup>Pb, in lake Pavin in many ways resembles that in the ocean, only the time scales of the processes involved are faster.</p></div>","PeriodicalId":100231,"journal":{"name":"Chemical Geology: Isotope Geoscience section","volume":"94 3","pages":"Pages 173-181"},"PeriodicalIF":0.0000,"publicationDate":"1992-03-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0168-9622(92)90010-8","citationCount":"3","resultStr":"{\"title\":\"210Pb, 226Ra and 32Si in Pavin lake (Massif Central, France)\",\"authors\":\"J-M. Martins, M. Meybecks , V.N. Nijampurkar , B.L.K. Somayajulu\",\"doi\":\"10.1016/0168-9622(92)90010-8\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Measurements of cosmogenic <sup>32</sup>Si and the U-decay series' nuclides <sup>210</sup>Ph and <sup>226</sup>Ra in waters and sediments of lake Pavin are reported. Both <sup>210</sup>Pb and <sup>226</sup>Ra are enriched in the anoxic deep waters compared to the oxic surface waters, respectively by a factor of 4 and 10, whereas <sup>32</sup>Si is depleted by a factor of ∼ 2. Redox conditions in the lake appear to have no marked effect on the <sup>32</sup>Si. Using a steady-state box model it is shown that the deep-water <sup>32</sup>Si concentration is controlled by the underground lacustrine springs. The residence times of <sup>210</sup>Pb, <sup>32</sup>Si and <sup>226</sup>Ra are ∼ 1, ∼ 10 and ∼ 80 a, respectively. In the case of <sup>32</sup>Si where more data are available, the assessed inventory data from the overhead atmospheric fallout and that measured in the sediments agree very well as expected. The <sup>210</sup>Pb, and <sup>32</sup>Si-based deposition rates during the past ∼ 100 a ranged from 0.8 to 1.9 mm a<sup>−1</sup>, earlier these were a factor of ∼ 3–5 faster. The geochemistry of <sup>32</sup>Si and <sup>210</sup>Pb, in lake Pavin in many ways resembles that in the ocean, only the time scales of the processes involved are faster.</p></div>\",\"PeriodicalId\":100231,\"journal\":{\"name\":\"Chemical Geology: Isotope Geoscience section\",\"volume\":\"94 3\",\"pages\":\"Pages 173-181\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1992-03-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0168-9622(92)90010-8\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chemical Geology: Isotope Geoscience section\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/0168962292900108\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chemical Geology: Isotope Geoscience section","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0168962292900108","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3
摘要
报道了帕文湖水体和沉积物中宇宙成因32Si和铀衰变系列核素210Ph和226Ra的测量结果。与富氧地表水相比,缺氧深水中210Pb和226Ra的富集程度分别是富氧水体的4倍和10倍,而32Si的富集程度是富氧水体的2倍。湖中的氧化还原条件似乎对32Si没有明显的影响。利用稳态箱形模型分析表明,深水区32Si浓度受地下湖泉水控制。210Pb、32Si和226Ra的停留时间分别为~ 1、~ 10和~ 80 a。在可获得更多数据的32Si的情况下,来自头顶大气沉降物的评估清单数据与沉积物中测量的数据非常符合预期。在过去的~ 100 a期间,210Pb和32si的沉积速率从0.8到1.9 mm a−1不等,在此之前,这些速率是一个因子~ 3-5。Pavin湖中32Si和210Pb的地球化学特征在很多方面与海洋中的相似,只是相关过程的时间尺度更快。
210Pb, 226Ra and 32Si in Pavin lake (Massif Central, France)
Measurements of cosmogenic 32Si and the U-decay series' nuclides 210Ph and 226Ra in waters and sediments of lake Pavin are reported. Both 210Pb and 226Ra are enriched in the anoxic deep waters compared to the oxic surface waters, respectively by a factor of 4 and 10, whereas 32Si is depleted by a factor of ∼ 2. Redox conditions in the lake appear to have no marked effect on the 32Si. Using a steady-state box model it is shown that the deep-water 32Si concentration is controlled by the underground lacustrine springs. The residence times of 210Pb, 32Si and 226Ra are ∼ 1, ∼ 10 and ∼ 80 a, respectively. In the case of 32Si where more data are available, the assessed inventory data from the overhead atmospheric fallout and that measured in the sediments agree very well as expected. The 210Pb, and 32Si-based deposition rates during the past ∼ 100 a ranged from 0.8 to 1.9 mm a−1, earlier these were a factor of ∼ 3–5 faster. The geochemistry of 32Si and 210Pb, in lake Pavin in many ways resembles that in the ocean, only the time scales of the processes involved are faster.