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The radiative impact of desert dust on orographic rain in the Cevennes-Vivarais area: a case study from HyMeX

机译:沙漠粉尘对Cevennes-Vivarais地区的地形雨的辐射影响 - 夏日快乐的案例研究

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摘要

The study is focused on Intensive Observation Period (IOP) 14 of the Hydrological Cycle in the Mediterranean Experiment first Special Observing Period (HyMeX SOP 1) that took place from 17 to 19 October 2012 and was dedicated to the study of orographic rain in the Cevennes-Vivarais (CV) target area. During this IOP a dense dust plume originating from northern Africa (the Maghreb and Sahara) was observed to be transported over the Balearic Islands towards the south of France. The plume was characterized by an aerosol optical depth between 0.2 and 0.8 at 550 nm, highly variable in time and space over the western Mediterranean Basin. The impact of this dust plume, the biggest event observed during the 2-month-long HyMeX SOP 1, on the precipitation over the CV area has been analyzed using high-resolution simulations from the convection permitting mesoscale model Meso-NH (mesoscale non-hydrostatic model) validated against measurements obtained from numerous instruments deployed specifically during SOP 1 (ground-based/airborne water vapor and aerosol lidars, airborne microphysics probes) as well as space-borne aerosol products. The 4-day simulation reproduced realistically the temporal and spatial variability (including the vertical distribution) of the dust. The dust radiative impact led to an average 0.6K heating at the altitude of the dust layer in the CV area (and up to +3K locally) and an average 100 Jkg(-1) increase of most unstable convective available potential energy (and up to +900J kg(-1) locally) with respect to a simulation without prescribed dust aerosols. The rainfall amounts and location were only marginally affected by the dust radiative effect, even after 4 days of simulation. The transient nature of this radiative effect in dynamical environments such as those found in the vicinity of heavy precipitation events in the Mediterranean is not sufficient to impact 24 h of accumulated rainfall in the dust simulation.
机译:该研究专注于地中海实验中的水文循环的强烈观察期(IOP)14,首先从2012年10月17日至19日发生的第一个特殊观察期(Hymex SOP 1),并致力于在Cevennes中的地形雨中研究-vivarais(CV)目标区域。在此期间,观察到源自北非(Maghreb和Sahara)的密集灰尘被观察到在法国南部的巴利阿里群岛上运输。该羽流的特征在于气溶胶光学深度0.2至0.8的550nm,时间和空间在西部地中海盆地的空间高度变化。使用来自CV区域的2个月长的Hymex SOP 1期间观察到的最大事件的影响已经使用来自CV地区的降水,从对流允许的Meso-NH(Mesoscale非 - 静水压模型)验证了从SOP 1(基于地面/空气蒸汽和气溶胶LIDARS,空气传播的气溶胶产品)专门部署的许多仪器获得的测量测量。为期4天的模拟重现了灰尘的时间和空间变异性(包括垂直分布)。灰尘辐射冲击导致CV区域(局部最多+ 3K)的灰尘层的海拔高度平均0.6K加热,平均100 JKG(-1)增加最不稳定的对流可用潜在能量(和上升)关于+ 900J kg(-1)本地)关于没有规定粉尘气溶胶的模拟。降雨量和位置甚至在仿真4天后的尘埃辐射效果略微影响。动态环境中这种辐射效果的瞬态性质,例如在地中海的重度降水事件附近发现的那些的辐射性质不足以影响粉尘模拟中的24小时累积降雨。

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