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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Thorium isotopes in the western Mediterranean Sea: an insight into the marine particle dynamics
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Thorium isotopes in the western Mediterranean Sea: an insight into the marine particle dynamics

机译:地中海西部的同位素:对海洋粒子动力学的认识

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We present a detailed view of the ~(23)Th-~(232)Th systematics in the western Mediterranean Sea in order to constrain water and particle fluxes. The conclusions obtained at the regional scale are also relevant at a more global scale although they may be more difficult to establish in the open ocean. ~(23)Th and ~(232)Th were analyzed in size-fractionated seawater and marine particle samples collected in the Ligurian, Alboran and Ionian seas. The ~(23)Th_(xs) (~(23)Th produced by the radioactive decay of ~(234)U in seawater) profiles at DYFAMED and in the Alboran sea site are not linear due to the formation of deep waters. The difference of ~(23)Th_(xs) concentration between these two sites is related to the aging of the water masses and to different scavenging conditions. The ~(230)Th/~(232)Th ratio is used as a tracer during mixing processes to provide information on the pathways followed by the matter in the water column. At DYFAMED, filtered (<0.2 μm) and ultrafiltered (<1 kDa) solutions have similar ~(23)Th/~(232)Th ratios, suggesting that an equilibrium exists between truly dissolved and colloidal Th. The change of the Th flux and of the ~(23)Th/~(232)Th ratio of trapped particles observed in August between 200 m and 1000 m is best explained by aggregation of filtered large particles on the trapped particles. The residence time of filtered large particles with respect to aggregation on trapped particles is of the order of 8-80 days. The combined budget of ~(23)Th and ~(232)Th inputs to the western Mediterranean Sea requires the dissolution of 3-5% of the Th associated with all the continental particulate inputs (including particles sequestered in margins) suggesting that eolian inputs are not the only source of refractory elements to the Mediterranean Sea and may be to the whole ocean.
机译:为了限制水和颗粒通量,我们提出了地中海西部〜(23)Th-〜(232)Th系统学的详细视图。尽管在公开海洋中可能难以确定,但在区域范围内得出的结论在全球范围内也具有相关性。在利古里亚海,阿尔伯兰海和爱奥尼亚海中收集的大小分离的海水和海洋颗粒样品中分析了〜(23)Th和〜(232)Th。 DYFAMED和阿尔伯兰海站点的〜(23)Th_(xs)(〜(23)Th由海水中〜(234)U的放射性衰变产生)剖面由于形成深水而呈非线性。这两个位置之间〜(23)Th_(xs)浓度的差异与水团的老化和不同的清除条件有关。 〜(230)Th /〜(232)Th比率在混合过程中用作示踪剂,以提供有关水柱中物质所遵循的路径的信息。在DYFAMED时,过滤后的(<0.2μm)和超过滤后的(<1 kDa)溶液具有相似的〜(23)Th /〜(232)Th比率,这表明在真正溶解的胶态Th和胶态Th之间存在平衡。八月份观察到的200 m至1000 m之间的Th通量和〜(23)Th /〜(232)Th比率的变化最好通过过滤后的大颗粒聚集在捕获的颗粒上来解释。相对于聚集在捕获的颗粒上,过滤的大颗粒的停留时间约为8-80天。向西地中海投入的〜(23)Th和〜(232)Th的总预算要求将与所有大陆颗粒物输入(包括隔离在边际中的颗粒物)相关的Th的3-5%溶解掉,这表明风积物输入并非地中海耐火元素的唯一来源,而且可能是整个海洋的耐火元素。

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