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Rapid changes of dust geochemistry in the Saharan Air Layer linked to sources and meteorology

机译:撒哈拉沙漠大气层中尘埃地球化学的快速变化与来源和气象有关

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Based at Izafia Observatory (-2400 m a.s.l. in Tenerife), we performed 1-h resolution measurements of elemental composition of dust in the Saharan Air Layer (SAL) and studied the variability of the ratios of these elements to aluminium (elemental ratios). In a period (-1 week) of continuous dust presence (50-200 pg/m3), we observed rapid variations of dust composition; some elemental ratios changed by a factor 2 in a few (5-8) hours. The lowest variability (Normalized Variability Range, %) was found for Si/A1 (9%) and Fe/A1 (9%), followed by the ratios of K, Ti, Mg, Mn, Ca and Sr to Al (20-80%), and the highest for S/Al, Na/Al and Cl/A1 (110-160%) and a number of trace metals (Cr, Cu, Ni, Zn, Zr) and Br (>200%). This variability was induced by the alternating impacts of three of the large North African dust sources: NE Algeria (rich in evaporite minerals bearing Ca, S, Sr, K and Mg and in illite mineral), Western Sahara to Bechar region (containing Na, S and Cl rich Yermosol soils) and SW Sahara Western Sahel (rich in illite and hematite). We traced the variability in large-scale meteorology using the so-called North African Dipole Intensity (NAFDI: strength of the subtropical Saharan high -Morocco-to the monsoon tropical low -Nigeria-). The mobilization of dust from the different sources was associated with westward propagating Harmattan pulses linked to the change of phase of NAFDI (- to +), the associated westward shifts of the Saharan Heat Low and convective monsoon inflow. We found a correlation between dust composition in the SAL and NAFDI: moderate NAFDI values (0 to +2.5) were associated with Ca, K, Na, Mg and S rich dust linked to dust sources in NE Algeria, whereas higher NAFDI values (+2.5 to +4) were linked to Fe rich dust (Ca, Na and S depleted) linked to dust sources in SW Sahara - Western Sahel. The results of this study also show that some trace elements (Br, Cr, Ni, Zn and Zr) are influenced by industrial emissions into North Africa.
机译:我们以伊扎菲亚天文台(特内里费岛-2400 m.s.l.)为基地,对撒哈拉沙漠空气层(SAL)中尘埃的元素组成进行了1小时的分辨率测量,并研究了这些元素与铝的比率(元素比率)的变化性。在连续存在粉尘(50-200 pg / m3)的时间段(-1周)中,我们观察到粉尘成分快速变化。一些元素比例在几(5-8)个小时内变化了2倍。发现Si / A1(9%)和Fe / A1(9%)的最低变异性(归一化变异范围,%),然后是K,Ti,Mg,Mn,Ca和Sr与Al的比率(20- 80%),最高的是S / Al,Na / Al和Cl / Al(110-160%)以及多种痕量金属(Cr,Cu,Ni,Zn,Zr)和Br(> 200%)。这种变异性是由北非三个大型粉尘源的交替影响引起的:东北阿尔及利亚(富含Ca,S,Sr,K和Mg的蒸发矿物和伊利石矿物),西撒哈拉至Bechar地区(含Na, S和Cl富含耶尔莫索尔土壤)和SW撒哈拉沙漠西部Sahel(富含伊利石和赤铁矿)。我们使用所谓的北非偶极子强度(NAFDI:亚热带撒哈拉以高摩洛哥的强度到季风热带低以尼日利亚的强度)来追踪大规模气象的变化。来自不同来源的粉尘的集结与向西传播的Harmattan脉冲有关,该脉冲与NAFDI的相变(从-到+),撒哈拉低热和向对流的季风流入有关。我们发现SAL和NAFDI中的粉尘成分之间存在相关性:中度NAFDI值(0至+2.5)与与阿尔及利亚东北部粉尘源相关的富含Ca,K,Na,Mg和S的粉尘相关,而较高的NAFDI值(+ 2.5至+4)与西南撒哈拉西部撒哈拉沙漠中的尘埃源有关的富铁尘埃(Ca,Na和S耗尽)。这项研究的结果还表明,一些微量元素(Br,Cr,Ni,Zn和Zr)受向北非工业排放的影响。

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