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Analysis of intense dust storms over the eastern Mediterranean in March 2018: Impact on radiative forcing and Athens air quality

机译:2018年3月地中海东部强烈沙尘暴的分析:对辐射强迫和雅典空气质量的影响

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This study examines the multiple dust storms that hit the eastern Mediterranean and Greece during March 2018, emphasizing on the atmospheric dynamics for their generation, the source regions, the dust-induced radiative forcing and the impacts on PM concentrations in Athens. In March 2018, several dust storms facilitated by increased cyclonicity in the western Europe/Mediterranean and by the Sharav cyclogenesis along the north African coast resulted in abnormal-high columnar aerosol loading and PM concentrations over Greece. The dusty days were associated with intense winds ( 15 . 20 ms(-1)) from southwestern directions, triggered by cyclonic circulations over the central/eastern Mediterranean and troughs over Italy and the north African coast. Statistical analysis of the backward air-mass trajectories shows that the highest PM10 concentrations are related to dust sources in Libya, while Ceilometer profiles indicate thick dust plumes with highest intensity between the surface and 3 km over Athens. The monthly-averaged hourly PM 10 concentrations at several stations in the Athens basin ranged from 37 mu gm(-3) to 53 mu gm(-3), while nine days exhibited PM 10 daily-means above 50 mu gm(-3), characterized as dusty days. The PM10 concentrations in Athens maximized on 25-26 March (similar to 500 mu gm(-3) at hourly basis), while the PM2.5 constitutes 38%-59% of PM 10 , indicating a dominance of coarse particles. Aerosol radiative forcing (ARF) estimates via the synergy of OPAC and SBDART models at three AERONET stations in Greece revealed significant impact of dust on radiation budget, with large (similar to- 40 W m(-2) to -50 W m(-2)) decrease in surface solar radiation and an overall cooling effect at the top of atmosphere (similar to - 5 to - 30 W m(-2)). The atmospheric heating via the dust-aerosol absorption results in heating rates of similar to 0.5 K day(-1).
机译:这项研究调查了2018年3月袭击地中海东部和希腊的多场沙尘暴,着重介绍了其产生的大气动力学,源区域,粉尘引起的辐射强迫以及对雅典PM浓度的影响。 2018年3月,西欧/地中海气旋强度增加以及北非海岸的Sharav气旋作用促进了几场沙尘暴,导致希腊上空的柱状气溶胶含量和PM浓度异常高。尘土飞扬的日子与西南方向的强风(> 15。20 ms(-1))有关,这是由于地中海中部/东部的旋风环流以及意大利和北非海岸的低谷引发的。后向空气质量轨迹的统计分析表明,最高的PM10浓度与利比亚的粉尘源有关,而云高仪的分布图表明,地表至雅典上方3公里之间的尘埃羽很浓,强度最高。雅典盆地几个站点的每月平均PM 10每小时浓度范围从37μgm(-3)到53 mugm(-3),而9天的PM 10日均值则高于50μgm(-3)。 ,特点是尘土飞扬的日子。雅典的PM10浓度在3月25日至26日达到最高(按小时计约为500μgm(-3)),而PM2.5则占PM 10的38%-59%,表明粗颗粒占主导地位。通过希腊三个AERONET站的OPAC和SBDART模型的协同作用得出的气溶胶辐射强迫(ARF)估算显示,粉尘对辐射预算具有重大影响,其影响较大(类似于-40 W m(-2)至-50 W m(- 2))减少了表面太阳辐射并降低了大气层顶部的整体冷却效果(类似于-5至-30 W m(-2))。通过粉尘气溶胶吸收进行的大气加热导致加热速率接近0.5 K天(-1)。

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