罗马尼亚蒂米什瓦拉太阳辐射的光谱特征

Sergiu Hațegan, M. Paulescu
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引用次数: 0

摘要

本文研究了罗马尼亚蒂米什瓦拉地区太阳辐射的光谱分布。根据Leckner的光谱太阳辐照度模型和2019-2020年测量的大气参数估算了地面的太阳光谱。利用平均光子能量指数(APE)捕捉太阳辐射光谱的特征特征。结果强调了蒂米什瓦拉太阳辐射光谱与标准AM1.5G光谱之间的巨大差异。在2019-2020年期间,APE的值在1.841 eV和1.929 eV之间,表明从标准AM1.5G光谱中红移和蓝移。据我们所知,这是第一次在罗马尼亚某地讨论太阳辐射光谱的APE特征的研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spectral Characteristics of Solar Radiation in Timisoara, Romania
Abstract This study deals with the spectral distribution of solar radiation in Timisoara, Romania. Solar spectrum at the ground level was estimated based on Leckner’s spectral solar irradiance model and measured atmospheric parameters over the years 2019-2020. The average photon energy index (APE) was used to capture the characteristic signature of the solar radiation spectrum. The results emphasize considerable differences between the solar radiation spectrum in Timisoara and the standard AM1.5G spectrum. During 2019-2020, APE has taken values between 1.841 eV and 1.929 eV, indicating both red- and blue-shift from the standard AM1.5G spectrum. To our best knowledge this is the first study which discusses the signature of solar radiation spectrum in terms of APE for a location in Romania.
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