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Influence of the vertical absorption profile of mixed Asian dust plumes on aerosol direct radiative forcing over East Asia

机译:亚洲混合粉尘羽垂直吸收剖面对东亚气溶胶直接辐射强迫的影响

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We estimate the aerosol direct radiative forcing (ADRF) and heating rate profiles of mixed East Asian dust plumes in the solar wavelength region ranging from 0.25 to 4.0 mu m using the Santa Barbara Discrete Ordinate Atmospheric Radiative Transfer (SBDART) code. Vertical profiles of aerosol extinction coefficients and single-scattering albedos (SSA) were derived from measurements with a multi-wavelength Raman lidar system. The data are used as input parameters for our radiative transfer calculations. We considered four cases of radiative forcing in SBDART: 1. dust, 2. pollution, 3. mixed dust plume and the use of vertical profiles of SSA, and 4. mixed dust plumes and the use of column-averaged values of SSA. In our sensitivity study we examined the influence of SSA and aerosol layer height on our results. The ADRF at the surface and in the atmosphere shows a small dependence on the specific shape of the aerosol extinction vertical profile and its light-absorption property for all four cases. In contrast, at the top of the atmosphere (TOA), the ADRF is largely affected by the vertical distribution of the aerosols extinction. This effect increases if the light-absorption capacity (decrease of SSA) of the aerosols increases. We find different radiative effects in situations in which two layers of aerosols had different light-absorption properties. The largest difference was observed at the TOA for an absorbing aerosol layer at high altitude in which we considered in one case the vertical profile of SSA and in another case the column-averaged SSA only. The ADRF at the TOA increases when the light-absorbing aerosol layer is located above 3 km altitude. The differences between height-resolved SSA, which can be obtained from lidar data, and total layer-mean SSA indicates that the use of a layer-mean SSA can be rather misleading as it can induce a large error in the calculation of the ADRF at the TOA, which in turn may cause errors in the vertical profiles of heating rates. (C) 2016 Elsevier Ltd. All rights reserved.
机译:我们使用圣塔芭芭拉离散普通垂直大气辐射传输(SBDART)代码估算了太阳波长范围为0.25至4.0μm的混合东亚尘埃羽流的气溶胶直接辐射强迫(ADRF)和加热速率分布。气溶胶消光系数和单散射反照率(SSA)的垂直剖面是通过多波长拉曼激光雷达系统的测量得出的。数据用作我们的辐射传递计算的输入参数。我们考虑了SBDART中的四种辐射强迫情况:1.灰尘,2。污染,3.混合尘埃羽和使用SSA的垂直剖面,以及4.混合尘埃羽和使用SSA的列平均值。在我们的敏感性研究中,我们检查了SSA和气溶胶层高度对我们结果的影响。在所有四种情况下,地表和大气中的ADRF都对气溶胶消灭垂直剖面的特定形状及其光吸收特性显示出很小的依赖性。相反,在大气层(TOA)的顶部,ADRF受到气溶胶绝灭的垂直分布的很大影响。如果气溶胶的光吸收能力(SSA降低)增加,则该效果会增强。在两层气溶胶具有不同的光吸收特性的情况下,我们发现了不同的辐射效应。在高海拔地区,在TOA上观察到最大的吸收气溶胶层差异,在这种情况下,我们在一种情况下仅考虑SSA的垂直剖面,而在另一种情况下仅考虑列平均SSA。当吸光气溶胶层位于海拔3 km以上时,TOA处的ADRF增加。可以从激光雷达数据获得的高度分辨的SSA与总层均值SSA之间的差异表明,使用层均值SSA可能会引起误解,因为它会在计算ADRF时引起较大误差。 TOA,这反过来可能导致加热速率的垂直分布中的错误。 (C)2016 Elsevier Ltd.保留所有权利。

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