Spectral measurements of aerosol particle extinction in the 0.4–3.7 μm wavelength range, performed at Sagres with the IR‐RAD sun‐radiometer

IF 2.3 4区 地球科学 Q3 METEOROLOGY & ATMOSPHERIC SCIENCES
V. Vitale, C. Tomasi, W. V. Hoyningen-Huene, U. Bonafè, S. Marani, A. Lupi, A. Cacciari, P. Ruggeri
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引用次数: 15

Abstract

During the CLEARCOLUMN campaign which took place at Sagres (Portugal) from 16 June to 25 July 1997, more than 2000 spectral measurements of direct solar irradiance were performed at thirteen window-wavelengths in the 0.4–3.7 μm range, on 27 days. The measurements were performed using the IR-RAD sun-radiometer designed and manufactured at the Institute ISAO (FISBAT), Bologna (Italy), and carefully calibrated by applying the Langley plot method to the measurements performed on 24 October 1996, at the Schneefernerhaus Observatory on the Zugspitze (Germany). From these measurements, the values of the total atmospheric optical depth were obtained at the various wavelengths, from which the corresponding spectral values of aerosol optical depth were determined through accurate corrections for Rayleigh scattering and gaseous absorption. Such values were found to be mostly smaller than 0.1 during June and early July, presenting almost neutral spectral dependence characteristics, closely related to the prevailing oceanic origins of particulate matter. Higher values of aerosol optical thickness, mainly ranging between 0.1 and 0.5 at visible wavelengths and sharply decreasing with wavelength, were found during the rest of July in the presence of predominant contents of continental and anthropogenic aerosol particles arriving from polluted European regions. The King inversion method was applied to the spectral series of aerosol optical depth to determine the particle size-distribution curves in the 0.2–20 μm diameter range. For 2 of these cases (one chosen for a low atmospheric loading of marine aerosols and the other for a mean content of continental/anthropogenic aerosols), the changes in the outgoing solar radiation flux produced by aerosol particles were calculated, considering different surface albedo conditions. The results obtained in the second case show that changes of opposite sign can be caused by the same atmospheric aerosol loading when passing from oceanic to continental areas.
在Sagres用IR - RAD太阳辐射计测量0.4-3.7 μm波长范围内气溶胶粒子消光的光谱
在1997年6月16日至7月25日在Sagres(葡萄牙)进行的CLEARCOLUMN活动期间,在27天内对0.4-3.7 μm范围内的13个窗口波长进行了2000多次直接太阳辐照度的光谱测量。测量是使用博洛尼亚(意大利)ISAO研究所(FISBAT)设计和制造的IR-RAD太阳辐射计进行的,并在1996年10月24日在Zugspitze(德国)的Schneefernerhaus天文台进行的测量中采用兰利图法进行了仔细校准。通过这些测量,获得了不同波长下的大气总光学深度值,并通过对瑞利散射和气体吸收的精确校正,确定了相应的气溶胶光学深度光谱值。在6月和7月初,这些值大多小于0.1,呈现出几乎中性的光谱依赖特征,与主要的海洋颗粒物来源密切相关。在7月其余时间,来自欧洲污染地区的大陆气溶胶粒子和人为气溶胶粒子的含量占主导地位,气溶胶光学厚度较高,主要在可见光波长范围在0.1至0.5之间,随波长急剧下降。将King反演方法应用于气溶胶光学深度光谱序列,确定0.2 ~ 20 μm直径范围内的粒径分布曲线。对于其中的2种情况(一种选择为海洋气溶胶的低大气负荷,另一种选择为大陆/人为气溶胶的平均含量),考虑不同的地表反照率条件,计算了气溶胶颗粒产生的太阳辐射通量的变化。在第二种情况下得到的结果表明,相同的大气气溶胶载荷从海洋到大陆地区时,可以引起相反的符号变化。
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期刊介绍: Tellus B: Chemical and Physical Meteorology along with its sister journal Tellus A: Dynamic Meteorology and Oceanography, are the international, peer-reviewed journals of the International Meteorological Institute in Stockholm, an independent non-for-profit body integrated into the Department of Meteorology at the Faculty of Sciences of Stockholm University, Sweden. Aiming to promote the exchange of knowledge about meteorology from across a range of scientific sub-disciplines, the two journals serve an international community of researchers, policy makers, managers, media and the general public.
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