首页> 外文OA文献 >Ground/satellite observations and atmospheric modeling of dust storms originating in the high Puna-Altiplano deserts (South America): Implications for the interpretation of paleo-climatic archives
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Ground/satellite observations and atmospheric modeling of dust storms originating in the high Puna-Altiplano deserts (South America): Implications for the interpretation of paleo-climatic archives

机译:来自高普纳-高原沙漠(南美)的沙尘暴的地面/卫星观测和大气模型:对古气候档案解释的启示

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摘要

This study provides a detailed description of the sources, transport, dispersion, and deposition of two major dust events originating from the high‐altitude subtropical Puna‐Altiplano Plateau (15?26°S; 65?69°W) in South America. A long and severe drought provided the right conditions for the onset of both events in July 2009 and 2010. Dust was transported SE and deposited over the Pampas region and was observed to continue to the Atlantic Ocean. Dust monitoring stations located downwind recorded both events, and samples were characterized through chemical and textural analysis. Through a combination of meteorological data and satellite observations (CALIPSO andMODIS detectors), we estimate the emission flux for the 2010 event. This estimate was used to constrain the Hybrid Single Particle Lagrangian Integrated Trajectory (HYSPLIT) transport model and simulate the dust event. Both satellite imagery and model results agree in the location and extension of the dust cloud. CALIPSO detected dust between ~6000 and ~8500 m a.s.l., which remained at this height during most of its trajectory. The dust cloud mixed with a strong convective system in the region, and the associated precipitation brought down significant amounts of dust to the ground. Dust particle size analysis for both events indicates that near the sources dust samples show median modes of 12.4?14.1 μm, similar to modes observed 1300 km away. Chemical composition of sediments from potential dust sources shows distinct signatures within the Puna‐Altiplano Plateau, the Puna sector being clearly different from the Altiplano area. In addition, both sources are markedly different from the Patagonian chemical fingerprint.These results have important implications to improve the interpretation of aleoenvironmental archives preserved on the Argentine loess, Antarctic ice cores, and Southern Ocean marine sediments.
机译:这项研究详细描述了源自南美高海拔亚热带Puna-Altiplano高原(15?26°S; 65?69°W)的两个主要尘埃事件的来源,迁移,扩散和沉积。长时间严重的干旱为2009年7月和2010年这两个事件的发生提供了适当的条件。粉尘通过SE运到潘帕斯地区,并沉积在整个潘帕斯地区,并观察到继续向大西洋传播。位于顺风的粉尘监测站记录了这两个事件,并通过化学和质地分析对样品进行了表征。通过结合气象数据和卫星观测(CALIPSO和MODIS探测器),我们估算了2010年事件的排放通量。该估计值用于约束混合单粒子拉格朗日综合轨迹(HYSPLIT)传输模型并模拟尘埃事件。卫星图像和模型结果在尘埃云的位置和扩展方面都一致。 CALIPSO检测到约6000至8500 m a.s.l.的尘埃,该尘埃在其大部分轨迹中都保持在该高度。尘埃云与该区域强大的对流系统混合,伴随的降水使大量尘埃落到地面上。对这两个事件的粉尘粒度分析表明,在源头附近,粉尘样本的中值模式为12.4?14.1μm,类似于在1300 km处观察到的模式。来自潜在尘埃来源的沉积物的化学成分在Puna-Altiplano高原内表现出明显的特征,Puna区域与Altiplano区域明显不同。此外,这两种来源均与巴塔哥尼亚的化学指纹显着不同,这些结果对于改善对阿根廷黄土,南极冰芯和南大洋海洋沉积物中保存的人类环境档案的解释具有重要意义。

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