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Spectral optical atmospheric thickness dependence on the specific humidity in the presence of continental and maritime air masses

机译:在存在大陆和海洋气团的情况下,光谱光学大气厚度取决于比湿度

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Atmospheric and spectral solar irradiation data, measured at the Atmospheric Physics Laboratory of the University of Patras (38°17′N, 21°47′E, 64 m a.s.l.), are used to determine the water vapor dependence of the spectral optical atmospheric thickness. The amount of the atmospheric water vapor is being described by the atmospheric specific humidity. The values of the spectral optical atmospheric thickness are being regressed with the simultaneous values of the atmospheric specific humidity and on the wavelength of the spectral solar irradiation, during the occurrence of continental and maritime air masses. The data analysis indicates the decrease of spectral optical atmospheric thickness with increase of the wavelength of the solar beam irradiation and, mainly, the major role of the amount of atmospheric water vapor on the spectral optical atmospheric thickness due to continental or maritime aerosols. The water vapor interaction with the particles of the insoluble continental dust results to the partial wetting and growing of the dust particles. In the atmospheric specific humidity minimum, which is observed in the dry and cold season, the spectral optical atmospheric thickness is minimized with the prevalence of continental air mass. In the atmospheric specific humidity maximum, which is observed in the wet and warm season, the spectral optical atmospheric thickness is maximized with the continental air mass prevalence, too. The water vapor interaction with the soluble sea-salt crystals of maritime aerosol is opposite from this with the insoluble continental dust and results in the complete dissolution of the sea-salt crystals in the wet season. During the presence of maritime air masses, the included sea-salt aerosols are dissolved by the atmospheric water vapor and the spectral optical atmospheric thickness takes intermediate values in the near violet and visible spectral regions of the solar spectrum. The observational data analysis results in two families of regression curves of the spectral optical atmospheric thickness with the atmospheric specific humidity, one corresponding to the continental and one to the maritime aerosol. The aim of this work is the explanation of the physical phenomenon of the hot sunrays during some winter days and of the weak sunrays during summer days.
机译:在帕特雷大学大气物理实验室(38°17'N,21°47'E,64 m asl)上测量的大气和光谱太阳辐射数据用于确定光谱光学大气厚度的水蒸气依赖性。大气中水蒸气的量由大气中的比湿度来描述。在发生大陆和海洋气团期间,光谱光学大气厚度的值与大气比湿度的同时值以及光谱太阳辐射的波长同时回归。数据分析表明,光谱光学大气厚度随太阳光束辐照波长的增加而减小,并且主要是由于大陆或海洋气溶胶引起的大气水汽量对光谱光学大气厚度的主要作用。水蒸气与不溶性大陆粉尘颗粒的相互作用导致粉尘颗粒的部分润湿和生长。在干旱和寒冷季节观测到的最低大气特定湿度下,光谱光学大气厚度随大陆性空气质量的流行而最小化。在湿热季节观测到的最大大气特定湿度下,光谱光学大气厚度也随大陆空气质量的普及而最大化。水蒸气与海洋气溶胶的可溶海盐晶体的相互作用与不可溶的大陆粉尘相反,导致湿季海盐晶体的完全溶解。在存在海洋气团的情况下,所包含的海盐气溶胶被大气中的水蒸气溶解,并且光谱光学大气厚度在太阳光谱的近紫色和可见光谱区域中取中间值。观测数据分析得出光谱光学大气厚度与大气比湿度的两类回归曲线,一类对应于大陆,一类对应于海洋气溶胶。这项工作的目的是解释某些冬季炎热的阳光和夏季炎热的阳光的物理现象。

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