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Dust deposition in the eastern Indian Ocean: The ocean perspective from Antarctica to the Bay of Bengal

机译:印度洋东部的尘埃沉积:从南极洲到孟加拉湾的海洋视角

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摘要

Atmospheric deposition is an important but still poorly constrained source of trace micronutrients to the open ocean because of the dearth of in situ measurements of total deposition (i.e., wet?+?dry deposition) in remote regions. In this work, we discuss the upper ocean distribution of dissolved Fe and Al in the eastern Indian Ocean along a 95°E meridional transect spanning the Antarctic margin to the Bay of Bengal. We use the mixed layer concentration of dissolved Al in conjunction with empirical data in a simple steady state model to produce 75 estimates of total dust deposition that we compare with historical observations and atmospheric model estimates. Except in the northern Bay of Bengal where the Ganges-Brahmaputra river plume contributes to the inventory of dissolved Al, the surface distribution of dissolved Al along 95°E is remarkably consistent with the large-scale gradients in mineral dust deposition and multiple-source regions impacting the eastern Indian Ocean. The lowest total dust deposition fluxes are calculated for the Southern Ocean (66?±?60?mg?m?2?yr?1) and the highest for the northern end of the south Indian subtropical gyre (up to 940?mg?m?2?yr?1 at 18°S) and in the southern Bay of Bengal (2500?±?570?mg?m?2?yr?1). Our total deposition fluxes, which have an uncertainty on the order of a factor of 3.5, are comparable with the composite atmospheric model data of Mahowald et al. (2005), except in the south Indian subtropical gyre where models may underestimate total deposition. Using available measurements of the solubility of Fe in aerosols, we confirm that dust deposition is a minor source of dissolved Fe to the Southern Ocean and show that aeolian deposition of dissolved Fe in the southern Bay of Bengal may be comparable to that observed underneath the Saharan dust plume in the Atlantic Ocean.
机译:由于缺乏对偏远地区总沉积物(即湿法+干法沉积)的原位测量的缺乏,大气沉积物是向海洋开放的重要微量微量营养素来源,但仍然受制于此。在这项工作中,我们讨论了印度洋东部溶解的铁和铝在沿南极边缘至孟加拉湾的经纬度为95°E的子午线上的上层海洋分布。在简单的稳态模型中,我们将溶解的Al的混合层浓度与经验数据结合使用,以产生75次总尘埃沉积的估算值,并将其与历史观测值和大气模型估算值进行比较。除了在孟加拉湾北部恒河-布拉马普特拉河羽流有助于溶解铝的存量外,沿95°E的溶解铝的表面分布与矿物粉尘沉积和多源区的大尺度梯度显着一致。影响印度洋东部。计算得出南洋最低的总尘埃沉积通量(66?±?60?mg?m?2?yr?1),南印度副热带回旋管的北端最高(最高940?mg?m在18°S处为?2?yr?1),在孟加拉湾南部(2500?±?570?mg?m?2?yr?1)。我们的总沉积通量的不确定性约为3.5倍,与Mahowald等人的复合大气模型数据相当。 (2005年),但印度南部亚热带回旋模型可能低估了总沉积。利用现有的铁在气溶胶中溶解度的测量结果,我们确认粉尘沉积是向南大洋溶解的Fe的次要来源,并表明在孟加拉湾南部的溶解铁的风沙沉积可能与撒哈拉沙漠下观察到的相当。大西洋上的尘埃羽。

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