Solar and thermal radiative effects during the 2011 extreme desert dust episode over Portugal

被引:27
作者
Valenzuela, A. [1 ,3 ,4 ]
Costa, M. J. [2 ]
Guerrero-Rascado, J. L. [3 ,4 ]
Bortoli, D. [1 ]
Olmo, F. J. [3 ,4 ]
机构
[1] Univ Evora, Dept Fis, Inst Ciencias Terra, Inst Invest & Formacao Avancada, Evora, Portugal
[2] Univ Evora, Dept Fis, Inst Ciencias Terra, Escola Ciencias & Tecnol, Evora, Portugal
[3] Andalusian Inst Earth Syst Res IISTA CEAMA, Avda Mediterraneo S-N, Granada 18006, Spain
[4] Univ Granada, Fac Sci, Dept Appl Phys, Fuentenueva S-N, E-18071 Granada, Spain
关键词
Dust; Aerosol vertical profiles; EARLINET; AERONET; Forcing; SAHARAN DUST; SCATTERING PROPERTIES; OPTICAL-PROPERTIES; IBERIAN PENINSULA; AEROSOL; LIDAR; SURFACE; URBAN; SENSITIVITY; EXTINCTION;
D O I
10.1016/j.atmosenv.2016.10.037
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
This paper analyses the influence of the extreme Saharan desert dust (DD) event on shortwave (SW) and longwave (LW) radiation at the EARLINET/AERONET Evora station (Southern Portugal) from 4 up to 7 April 2011. There was also some cloud occurrence in the period. In this context, it is essential to quantify the effect of cloud presence on aerosol radiative forcing. A radiative transfer model was initialized with aerosol optical properties, cloud vertical properties and meteorological atmospheric vertical profiles. The intercomparison between the instantaneous TOA shortwave and longwave fluxes derived using CERES and those calculated Using SBDART, which was fed with aerosol extinction coefficients derived from the CALIPSO and lidar-PAOLI observations, varying OPAC dataset parameters, was reasonably acceptable within the standard deviations. The dust aerosol type that yields the best fit was found to be the mineral accumulation mode. Therefore, SBDART model constrained with the CERES observations can be used to reliably determine aerosol radiative forcing and heating rates. Aerosol radiative forcings and heating rates were derived in the SW (ARF(sw), AHR(Sw)) and LW (ARF(Lw), AHR(Lw)) spectral ranges, considering a cloud-aerosol free reference atmosphere. We found that AOD at 440 nm increased by a factor of 5 on 6 April with respect to the lower dust load on 4 April. It was responsible by a strong cooling radiative effect pointed out by the ARF(sw) value (-99 W/m(2) for a solar zenith angle of 60 degrees) offset by a warming radiative effect according to ARF(Lw) value (+21.9 W/m(2)) at the surface. Overall, about 24% and 12% of the dust solar radiative cooling effect is compensated by its longwave warming effect at the surface and at the top of the atmosphere, respectively. Hence, larger aerosol loads could enhance the response between the absorption and re-emission processes increasing the ARF(Lw) with respect to those associated with moderate and low aerosol loads. The unprecedented results derived from this work complement the findings in other regions on the modifications of radiative energy budget by the dust aerosols, which could have relevant influences on the regional climate and will be topics for future investigations. (C) 2016 The Authors. Published by Elsevier Ltd.
引用
收藏
页码:16 / 29
页数:14
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