A preliminary assessment of the spatial and temporal patterns of sand and dust storms over the Sahara

IF 2.7 Q2 MULTIDISCIPLINARY SCIENCES
Sahar A. Saleh , Saleh A․ S․ , Hesham Badawy
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引用次数: 0

Abstract

The Sahara Desert, the preeminent global producer of airborne dust, is crucial for comprehending the geographical and temporal dynamics of sand and dust storms (SDSs), especially as climate change and anthropogenic activities exacerbate desertification. This study offers a spatiotemporal analysis of SDSs in the Sahara from 2000 to 2020, incorporating 2196 daily satellite observations from NASA’s Giovanni and POWER platforms alongside GIS-based regional clustering. We evaluated changes in SDS frequency, intensity, duration, and distribution over the past two decades. This study identified primary dust source locations, such as the Bodélé Depression, Western Sahara, and Libyan-Algerian sand seas, where geomorphological and atmospheric circumstances enable continuous dust emissions. A clear latitudinal gradient in dust activity was observed, with maximum aerosol optical thickness (AOT) occurring between 17° and 20°N, mostly corresponding to the yearly movement of the Intertropical Convergence Zone (ITCZ). However, there is a notable migration of dust deposition centers northward during warm seasons (summer and autumn) and shift southward toward the southern Sahara and West Africa during cold seasons (winter and spring). The results also reveal a statistically significant long-term reduction in SDS frequency, intensity, and duration, ascribed to enhanced Sahelian vegetation, diminishing wind patterns, and changing climate oscillations. In contrast, winter exhibited an increase in SDS activity, perhaps influenced by synoptic-scale meteorological phenomena such as high-pressure anomalies. Overall, the study's methodological framework, which integrates remote sensing and spatial analytics, improves the identification and monitoring of dust sources, thereby can contribute to improving models about radiative forcing, air quality, and transboundary dust movement. Policy implications necessitate the implementation of land management methods to mitigate dust emissions, in conjunction with early warning systems for health and climate adaptation.
撒哈拉沙漠沙尘暴时空格局的初步评估
撒哈拉沙漠是全球主要的空气尘埃产生地,对了解沙尘暴的地理和时间动态至关重要,特别是在气候变化和人为活动加剧荒漠化的情况下。本研究提供了2000年至2020年撒哈拉沙漠SDSs的时空分析,结合了来自NASA Giovanni和POWER平台的2196个每日卫星观测数据以及基于gis的区域聚类。我们评估了过去二十年中SDS频率、强度、持续时间和分布的变化。这项研究确定了主要的粉尘来源地点,如博德萨伊姆洼地、西撒哈拉和利比亚-阿尔及利亚沙海,那里的地貌和大气环境使粉尘持续排放。气溶胶光学厚度(AOT)最大值出现在17°~ 20°N之间,与热带辐合带(ITCZ)的年运动基本一致。然而,在温暖季节(夏季和秋季),沙尘沉降中心向北迁移,在寒冷季节(冬季和春季),沙尘沉降中心向南迁移到撒哈拉以南和西非。结果还显示,由于萨赫勒地区植被的增加、风型的减少和气候振荡的变化,SDS的频率、强度和持续时间在统计上有显著的长期减少。相反,冬季SDS活动增加,可能受到天气尺度气象现象(如高压异常)的影响。总体而言,该研究的方法框架结合了遥感和空间分析,改进了对沙尘源的识别和监测,从而有助于改进辐射强迫、空气质量和跨界沙尘运动的模式。政策方面的影响需要实施土地管理方法,以减少粉尘排放,并结合健康和气候适应预警系统。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Scientific African
Scientific African Multidisciplinary-Multidisciplinary
CiteScore
5.60
自引率
3.40%
发文量
332
审稿时长
10 weeks
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