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Optical properties of Saharan dust aerosol and contribution from the coarse mode as measured during the Fennec 2011 aircraft campaign

机译:在Fennec 2011飞机运动期间测量的撒哈拉沙尘气溶胶的光学特性和粗模式的贡献

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摘要

New in-situ aircraft measurements of Saharan dust originating from Mali, Mauritania and Algeria taken during the Fennec 2011 aircraft campaign over a remote part of the Sahara Desert are presented. Size distributions extending to 300 μm are shown, representing measurements extending further into the coarse mode than previously published for airborne Saharan dust. A significant coarse mode was present in the size distribution measurements with effective diameter (d) from 2.3 to 19.4 μm and coarse mode volume median diameter (d) from 5.8 to 45.3 μm. The mean size distribution had a larger relative proportion of coarse mode particles than previous aircraft measurements. The largest particles (with d > 12 μm, or d > 25 μm) were only encountered within 1 km of the ground. Number concentration, mass loading and extinction coefficient showed inverse relationships to dust age since uplift. Dust particle size showed a weak exponential relationship to dust age. Two cases of freshly uplifted dust showed quite different characteristics of size distribution and number concentration. Single Scattering Albed (SSA) values at 550 nm calculated from the measured size distributions revealed high absorption ranging from 0.70 to 0.97 depending on the refractive index. SSA was found to be strongly related to d. New instrumentation revealed that direct measurements, behind Rosemount inlets, overestimate SSA by up to 0.11 when d is greater than 2 μm. This is caused by aircraft inlet inefficiencies and sampling losses. Previous measurements of SSA from aircraft measurements may also have been overestimates for this reason. Radiative transfer calculations indicate that the range of SSAs during Fennec 2011 can lead to underestimates in shortwave atmospheric heating rates by 2.0 to 3.0 times if the coarse mode is neglected. This will have an impact on Saharan atmospheric dynamics and circulation, which should be taken into account by numerical weather prediction and climate models.
机译:提出了在Fennec 2011飞机战役期间在撒哈拉沙漠偏远地区进行的,来自马里,毛里塔尼亚和阿尔及利亚的撒哈拉沙漠尘土的新现场飞机测量。示出了扩展到300μm的尺寸分布,这些尺寸分布比以前发布的关于机载撒哈拉尘埃的测量进一步扩展到了粗模式。尺寸分布测量中存在明显的粗模式,有效直径(d)为2.3至19.4μm,粗模式体积中值直径(d)为5.8至45.3μm。平均尺寸分​​布具有比以前的飞机测量更大的粗模式颗粒相对比例。最大的颗粒(d> 12μm或d> 25μm)仅在距地面1 km内遇到。自隆起以来,数量浓度,质量负荷和消光系数与粉尘年龄呈反比关系。粉尘粒径与粉尘年龄之间呈弱指数关系。两例新近扬起的粉尘显示出大小分布和数量集中的特征完全不同。根据测得的尺寸分布计算出的550 nm处的单散射Albed(SSA)值显示出高吸收,范围从0.70到0.97,具体取决于折射率。发现SSA与d密切相关。新仪器显示,当d大于2μm时,直接测量在罗斯蒙特入口后面会导致SSA高估多达0.11。这是由于飞机进气口效率低下和采样损失所致。出于这个原因,以前根据飞机测量得出的SSA测量值也可能被高估了。辐射传递计算表明,如果忽略了粗模式,Fennec 2011期间的SSA范围可能导致短波大气加热速率低估2.0到3.0倍。这将对撒哈拉大气动力学和环流产生影响,数值天气预报和气候模型应考虑到这一点。

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