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Dissolved rare earth elements in the eastern Indian Ocean: chemical tracers of the water masses

机译:印度洋东部的溶解稀土元素:水团中的化学示踪剂

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摘要

New data on vertical profiles of dissolved rare earth elements (REEs) in the southeastern Indian Ocean are presented. The compositions of dissolved REEs are uniquely characterized by strong depletion in the light REEs; the extent of depletion decreasing systematically from La to Sm, as compared to those in the western Indian Ocean and the South Pacific. Dissolved Gd is also anomalously depleted in many of the water masses occupying this region. The LREE depleted patterns with a Gd deficit appear to be derived by input from volcanic sources around the Indonesian Archipelago, although the exact location and mechanism are not yet well understood. Nevertheless, the unique REE patterns can be used to trace the pathways of the water masses in the eastern Indian Ocean. The salinity minimum centered at ~1100 m at 40°S in the Antarctic Circumpolar region, southwest of Australia, can be considered as a boundary between the upper and the deeper layers, since the REE patterns around that depth are clearly different from those of the Antarctic Intermediate Water (AAIW) at 30°S on the Perth Basin and can be produced largely by mixing of the two waters. The unique REE patterns of AAIW with no significant Gd deficit between 497 and 2474 m in the Perth Basin indicate that the waters must be derived from somewhere else by lateral transport. The upper portion of the intermediate waters may be derived from a near-surface region in the Subantarctic zone, including the southernmost station in this study (40°S), and the deeper part may be contributed from the South Pacific reaching the area from south of Tasmania. The northward flow of the intermediate waters can be traced by the characteristic REE patterns at least to 10°S in the southeastern Indian Ocean, but does not reach the Bay of Bengal. The surface waters in the North Australia Basin have REE patterns similar to those of the surface waters in the western equatorial Pacific, suggesting a strong influence of Pacific waters to the region north of Australia. The light REE and Gd-deficient patterns are also found in the deep and bottom waters of the southeastern basins as well as in the surface waters from subtropical to temperate offshore regions, and they are presumably due to the influence of the Indonesian Archipelago. The unique pattern is clearly traced to the station at 40°S, 110°E, in the South Australia Basin, suggesting a southward flow of deep and bottom waters along the eastern edge of the Indian Ocean.
机译:提出了有关印度洋东南部溶解稀土元素(REE)垂直剖面的新数据。溶解的稀土元素的组成特征是轻稀土元素的强烈消耗。与印度洋西部和南太平洋相比,从La到Sm的耗竭程度有系统地降低。溶解的Gd在占据该区域的许多水团中也异常消耗。尽管尚未确切了解确切的位置和机制,但似乎有Gd缺陷的LREE枯竭模式是来自印度尼西亚群岛周围火山源的输入推导的。然而,独特的稀土元素模式可以用来追踪印度洋东部水团的路径。在澳大利亚西南极南极的极地地区,最低盐度以40°S〜1100 m为中心,可以认为是上层与深层之间的边界,因为该深度附近的REE模式明显不同于深部。珀斯盆地30°S的南极中间水(AAIW)可以通过将两种水混合而产生。珀斯盆地在497和2474 m之间没有明显的Gd赤字的AAIW独特的REE模式表明,这些水必须通过横向运输从其他地方获取。中间水的上部可能来自亚南极带的近地表区域,包括本研究中最南端的台站(40°S),而更深的部分可能是由南太平洋从南部到达该区域造成的。塔斯马尼亚州。在印度洋东南部至少有10°S的特征性REE模式可以追踪中间水域的北向流动,但没有到达孟加拉湾。北澳大利亚盆地的地表水的稀土元素分布与赤道西太平洋的地表水相似,表明太平洋水域对澳大利亚北部地区产生了强烈影响。在东南盆地的深水和底水以及亚热带到温带近海地区的地表水中也发现了轻稀土和G缺乏的模式,这大概是由于印度尼西亚群岛的影响。独特的模式清楚地追溯到南澳大利亚盆地中40°S,110°E的台站,表明印度洋东部边缘的深水和底水向南流动。

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