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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Numerical model simulation of the Saharan dust event of 6-11 March 2006 using the Regional Climate Model version 3 (RegCM3)
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Numerical model simulation of the Saharan dust event of 6-11 March 2006 using the Regional Climate Model version 3 (RegCM3)

机译:使用区域气候模型第3版(RegCM3)对2006年3月6日至11日的撒哈拉沙尘事件进行数值模拟

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摘要

The Sahara desert is the world's primary source of mineral dust aerosols and is known to be an important but poorly understood component of the climate system. Climate models which incorporate dust modules have the potential to improve our understanding of the climate impacts of dust. In this study, the performance of the Regional Climate Model version 3 (RegCM3) with an active dust scheme is evaluated, using a major dust event of 6-11 March 2006 as a test case. To account for the distribution of preferential dust source regions, soil texture characteristics were modified in dust source regions identified from long-term SEVIRI satellite data. The dust event was associated with a pronounced cold outbreak of midlatitude air over the northern Sahara which produced anomalously strong northerly winds, which propagated from west to east over the Sahara during the study period. This resulted in dust mobilization from multiple dust sources across the domain. RegCM3 represents the space/time structure of near-surface meteorology well, although surface winds are underestimated in absolute terms. The experiment in which soils are modified provides a better representation of local dust sources and emission and resulting atmospheric optical thickness (AOT). In this experiment, model simulated dust flux exported from the Sahara to the Sahel and the tropical east Atlantic is estimated as 1.9 Tg d~(-1). The dust event had a profound impact on the surface solar radiation budget of ~140 W m~(-20 per unit AOT (domain average). The shortwave radiative effect at the top of the atmosphere is ~-10 W m~(-2) per unit AOT over the study domain. However, this is strongly dependent on surface albedo. The results also highlight how errors in model simulated circulation lead to errors in the position of the dust plume.
机译:撒哈拉沙漠是世界上主要的矿物粉尘气溶胶来源,众所周知是气候系统的重要组成部分,但人们对其了解甚少。包含灰尘模块的气候模型有可能增进我们对灰尘对气候影响的理解。在本研究中,以2006年3月6日至11日的一次重大沙尘事件为例,对采用主动除尘方案的区域气候模型版本3(RegCM3)的性能进行了评估。为了考虑优先尘埃源区域的分布,对从SEVIRI长期卫星数据确定的尘埃源区域中的土壤质地特征进行了修改。沙尘事件与撒哈拉以北地区中纬度空气的明显爆发有关,产生了异常强烈的北风,在研究期间从北向西传播。这导致了整个域中多个尘埃源的尘埃动员。 RegCM3很好地代表了近地表气象学的时空结构,尽管从绝对意义上低估了地表风。改良土壤的实验可以更好地表示当地的粉尘源和排放,以及由此产生的大气光学厚度(AOT)。在该实验中,模型模拟的从撒哈拉沙漠输出到萨赫勒地区和热带东大西洋的粉尘通量估计为1.9 Tg d〜(-1)。尘埃事件对〜140 W m〜(每单位AOT -20(畴平均)的表面太阳辐射收支产生了深远的影响。大气层顶部的短波辐射效应为〜-10 W m〜(-2 )在研究范围内的每单位AOT,但这在很大程度上取决于地表反照率,结果还突显了模型模拟环流中的误差如何导致粉尘羽流位置的误差。

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