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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Accretion of Asian dust to Hawaiian soils: Isotopic, elemental, and mineral mass balances
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Accretion of Asian dust to Hawaiian soils: Isotopic, elemental, and mineral mass balances

机译:亚洲尘埃在夏威夷土壤上的吸积:同位素,元素和矿物质的质量平衡

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Hawaiian soils contain a mixture of material derived from in situ weathering of parent material plus atmospheric inputs, including sea salt aerosols and Asian dust. We use soil mineralogy and radiogenic isotope geochemistry (Sr and Nd) to evaluate the impact of Asian dust on a chronosequence of Hawaiian soils. Dust becomes an important constituent of soils 20 ky and older. Near-surface (< 50-cm depth) horizons contain as much as 30% quartz, a mineral absent from local parent material. Basaltic Sr and Nd isotope signatures in these horizons have been completely overprinted by Asian dust signatures, with Sr-87/Sr-86 ratios as high as 0.723 and epsilon (Nd) values as low as -7. REE patterns in these soils are indistinguishable from that of average upper continental crust. Quartz abundance and Nd isotopes provide two independent tracers of long-term dust additions to the chronosequence soils. The two tracers indicate a minimum long-term average dust accretion rate of 125 mg cm(-2) ky(-1) at the 150 ka chronosequence site, roughly a factor of three higher than Holocene dust accumulation rates estimated from North Pacific sediment cores. We find that the mass of dust preserved in these soil profiles does not increase with age in soils 150 ka and older, requiring a loss mechanism for accreted dust. On the basis of the geomorphic stability of these sites, observed preferential loss of dust-derived mica relative to quartz, and estimates of soil Si leaching rates we argue that chemical weathering is the dominant loss mechanism for dust from these soils. Dust has a profound effect on the budgets of elements that are susceptible to leaching losses. Dust becomes the dominant source of soil nutrients Si and P in the oldest, most intensely weathered soils. We calculate a dust-derived P input flux of 0.8 mg cm(-2) ky(-1), and a dust-derived Si input flux of 35 mg cm(-2) ky(-1). Si leaching fluxes are high (1400 mg cm(-2) ky(-1)) in the youngest (2 ka) soils and drop systematically with soil age to a value that closely balances the dust-derived Si input flux by 4100 ka. Extremely refractory elements such as Nb, which are concentrated in soils by residual enrichment processes, are much less readily impacted by dust addition. Although dust has had a pronounced impact on Sr and Nd isotopic budgets and on soil mineral composition at the 150 ka site, dust cannot have contributed >4% of the total Nb contained in this soil profile. Copyright (C) 2001 Elsevier Science Ltd. [References: 42]
机译:夏威夷的土壤中混合了多种物质,这些物质是由母体原位风化得到的,再加上大气成分,包括海盐气溶胶和亚洲粉尘。我们使用土壤矿物学和放射性同位素地球化学(Sr和Nd)来评估亚洲粉尘对夏威夷土壤的时间序列的影响。灰尘成为20 ky及以上土壤的重要成分。近地表(深度小于50厘米)的地层中含有多达30%的石英,这是当地母体材料中缺少的一种矿物。这些视野中的玄武质Sr和Nd同位素特征已被亚洲尘埃特征完全套印,Sr-87 / Sr-86比值高达0.723,ε(Nd)值低至-7。这些土壤中的REE模式与平均上陆壳没有区别。石英丰度和Nd同位素提供了两个独立的示踪剂,可以长期向年代序列土壤中添加粉尘。这两个示踪剂表明,在150 ka时序序列位点,最小长期平均粉尘积聚率为125 mg cm(-2)ky(-1),大约比根据北太平洋沉积物岩心估计的全新世粉尘积聚率高三倍。 。我们发现,在150 ka及以上的土壤中,保留在这些土壤剖面中的粉尘质量不会随着年龄的增长而增加,这需要一种用于沉积的粉尘的损失机制。根据这些站点的地貌稳定性,观察到相对于石英而言,粉尘云母的优先损失,以及土壤硅浸出率的估计,我们认为化学风化是这些土壤中粉尘的主要损失机制。灰尘对容易产生沥滤损失的元素的预算产生深远影响。在最古老,最强烈风化的土壤中,灰尘成为土壤养分Si和P的主要来源。我们计算得出,粉尘派生的P输入通量为0.8 mg cm(-2)ky(-1),粉尘派生的Si输入通量为35 mg cm(-2)ky(-1)。硅的淋溶通量在最年轻的(2 ka)土壤中很高(1400 mg cm(-2)ky(-1)),并且随着土壤年龄的增长而有系统地下降,其值与粉尘源的硅输入通量相差4100 ka。通过残留富集过程浓缩在土壤中的极难熔元素(例如Nb)受粉尘的影响不那么容易。尽管粉尘对Sr和Nd同位素的收支以及150 ka场地的土壤矿物质组成有显着影响,但粉尘不能贡献该土壤剖面中所含Nb的4%以上。版权所有(C)2001 Elsevier Science Ltd. [参考:42]

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