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Aerosol radiative effects during two desert dust events in August 2012 over the Southwestern Iberian Peninsula

机译:2012年8月西南伊比利亚半岛两次沙漠尘埃事件期间的气溶胶辐射效应

摘要

This study provides an analysis of desert dust aerosol radiative effects in the shortwave solar spectrum. For this purpose, the aerosol radiative forcing (ARF) at the earth's surface was calculated during two desert dust events that occurred during August 2012 over Badajoz (Spain) and Évora (Portugal), both stations are located in southwestern Iberian Peninsula. Aerosol properties from these two AERONET stations have been employed to feed the libRadtran model used to simulate irradiances in the shortwave range at the surface under cloud-free conditions. In addition, simulated irradiances for Évora have been compared with Eppley pyranometer measurements. Simulated irradiance values have been used to calculate ARF values at both sites. The overall mean simulated ARF values for Évora and Badajoz during the first event are − 43.03 and − 43.76 W m− 2, respectively, while, for the second event, the overall mean values are − 19.73 and − 26.07 W m− 2, respectively, indicating that the first event has a greater regional radiative impact than the second one, causing a more pronounced radiate cooling at the surface.The ARF per unit of aerosol optical depth (AOD), called the aerosol radiative forcing efficiency (ARFE), is also evaluated for this shortwave spectral range. The ARFE values obtained for Évora and Badajoz during the first event are − 112.93 ± 6.60 W m− 2 and − 101.63 ± 10.73 W m− 2 per unit of AOD (500 nm), respectively, and, for the second event, − 92.44 ± 9.82 W m− 2 and − 87.85 ± 10.19 W m− 2 per unit of AOD (500 nm), respectively. These values also confirm the previous results, i.e., the first event causes a greater radiate cooling than the second one in both stations, although the second desert dust event is more intense, i.e., with higher aerosol optical depth and PM10 aerosol mass concentration. The presence of absorbing aerosols, together with dust, near the surface during the first event may explain the greater efficiency of this aerosol mixture to reduce the downward shortwave irradiance reaching the surface, inducing a greater radiative cooling than the second event.
机译:这项研究提供了短波太阳光谱中沙漠尘埃气溶胶辐射效应的分析。为此,在2012年8月发生在巴达霍斯(西班牙)和埃沃拉(葡萄牙)的两次沙漠尘埃事件中,计算了地球表面的气溶胶辐射强迫(ARF),这两个站点均位于伊比利亚西南半岛。这两个AERONET站的气溶胶特性已被用于提供libRadtran模型,该模型用于模拟无云条件下表面短波范围内的辐照度。此外,已将埃弗拉的模拟辐照度与埃普利日射强度计测量值进行了比较。模拟辐照度值已用于计算两个站点的ARF值。第一次事件中Évora和Badajoz的总体平均模拟ARF值分别为− 43.03和− 43.76 W m-2,而第二次事件的总体均值分别为− 19.73和− 26.07 W m-2。表示第一个事件比第二个事件具有更大的区域辐射影响,从而在表面造成更明显的辐射冷却。每单位气溶胶光学深度(AOD)的ARF,称为气溶胶辐射强迫效率(ARFE)为还对该短波光谱范围进行了评估。在第一事件中为Évora和Badajoz获得的ARFE值分别为每单位AOD(500 nm)的− 112.93±6.60 W m-2和− 101.63±10.73 W m-2,第二事件为-92.44每单位AOD(500 nm)分别为±9.82 W m-2和− 87.85±10.19 W m-2。这些值也证实了先前的结果,即虽然第二次沙漠尘埃事件更为强烈,即具有更高的气溶胶光学深度和PM10气溶胶质量浓度,但两个站中的第一次事件都比第二次事件导致更大的辐射降温。在第一事件期间,在表面附近存在吸收性气溶胶以及灰尘,这可以解释这种气溶胶混合物降低到达表面的向下短波辐照度的更大效率,从而引起比第二事件更大的辐射冷却。

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