Prediction of Doses Biologically Active Ultraviolet Solar Radiation from Measurements of Global Solar Radiation

S. Khalil, U. A. Rahoma, A. Hassan, A. M. Shaffie
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Abstract

The ghastly scope of sun based radiation relating to frequencies λ< 400 nm, is called bright (UV). The bright is subdivided into three frequency band locales: the UV-A (315-400 nm) which is gotten at earth's surface, the UV-B (280-315 nm) which is halfway consumed by ozone or dispersed in the climate and UVC (<290 nm) which is possibly the most hazardous as it has the most elevated vitality levels, however this frequency band area is totally consumed by stratospheric ozone and oxygen above about 30km. Stratospheric ozone is known to be the most significant environmental factor deciding clear sky UV-B radiation arriving at the Earth's surface. The potential increment of UV-B presentation is the reason for mounting worry about the ozone layer. There are, be that as it may, different impacts that impact the UV brilliant vitality move: overcast spread, pressurized canned products, tropospheric ozone, and different vaporous toxins. The connections between different marvels occurring in the environment are perplexing. Along these lines, ground based UV estimations are important to investigate climatic changes and resultant impacts on the biosphere. The information on sun powered UV radiation arriving at the Earth's surface has an extraordinary intrigue due to its huge job in climatic and natural procedures. The UV-B sun based radiation (280-315 nm) speaks to ≈ 0.5% of the all-out radiation arriving at the earth surface, and it is significant for the Earth-living frameworks since it is a radiation of high vitality. UV-B irradiance on the Earth surface relies upon land factors, for example, scope, stature, earth-sun separation, and sunlight based peak edge (SZA), and so forth. The impact of these elements can be assessed utilizing distinctive radiative models. Anyway UV-B sunlight based radiation relies upon air parameters like ozone, mists and pressurized canned products. Ozone is the gas that ingests UVC and some UV-B sun powered radiation and the impact of the complete ozone segment was remembered for every single radiative model. Mists are Abstract: The main objective of this research, estimated of mean seasonal variations doses biologically active of UV-Bm solar radiation from global broadband solar irradiance over Egypt. The measurements of global solar radiation (G) and biologically effective erythematic radiation (EER) incident on a horizontal surface during the period time 1985 2015 at Cairo, Egypt are discussed. The monthly mean variation of slant ozone Z and UV-Bm transmission KtUV-B at the present work are found. The comparison between the two variables slant ozone Z and UV-Bm transmission KtUV-B are found. The seasonal statistical values of regression equations as the slopes (β), intercepts (α) and the standard errors (SE) for the fitted lines are done. The minimum slope occurs in winter, indicating that the percentage reduction in EER at higher slant ozone Z is larger than G. The variations of the slopes (β) during the year ranges from a minimum of 0.2867 in winter to a maximum of 0.3253 in summer, the intercepts also show their minimum and maximum values in cold humid and hot dry months. The temporal variability of the percentage ratio of the total hourly mean daily erythema to total hourly mean daily broadband solar global irradiation (EER/G) is presented. The estimated values of UV-Best solar radiation are a good agreement with the measured values of the UV-Bm solar radiation. The difference between the estimated and measured values of UV-B solar radiation varies from 3.1 to 4.25%.
从全球太阳辐射测量预测生物活性紫外线太阳辐射剂量
频率λ< 400nm的太阳辐射,被称为亮(UV)。明亮被细分为三个频段:UV-A(315-400纳米),从地球表面获得,UV-B(280-315纳米),一半被臭氧消耗或分散在气候中,UVC(<290纳米)可能是最危险的,因为它具有最高的活力水平,但是这个频段区域完全被平流层臭氧和氧气消耗。众所周知,平流层臭氧是决定晴空UV-B辐射到达地球表面的最重要环境因素。UV-B的潜在增加是人们越来越担心臭氧层的原因。尽管如此,影响紫外线活力的因素有很多:阴天、罐装产品、对流层臭氧和不同的蒸汽毒素。环境中发生的不同奇迹之间的联系令人困惑。沿着这些思路,地面紫外线估算对于研究气候变化及其对生物圈的影响是重要的。由于太阳辐射在气候和自然过程中起着巨大的作用,关于到达地球表面的太阳紫外线辐射的信息具有非凡的吸引力。基于太阳的UV-B辐射(280-315 nm)约占到达地球表面的总辐射的0.5%,由于它是一种高活力的辐射,因此对地球生命框架具有重要意义。地球表面的UV-B辐照度取决于陆地因素,如范围、高度、日地距离和基于太阳光的峰值边缘(SZA)等。这些因素的影响可以利用不同的辐射模式进行评估。无论如何,UV-B阳光辐射依赖于空气参数,如臭氧、雾和加压罐装产品。臭氧是吸收UVC和一些UV-B太阳辐射的气体,每一个单一的辐射模型都记住了完整臭氧部分的影响。摘要:本研究的主要目的是利用埃及的全球宽带太阳辐照度估算太阳辐射的平均季节变化剂量和生物活性。本文讨论了1985年至2015年期间在埃及开罗测量的全球太阳辐射(G)和入射在水平面上的生物有效红外辐射(EER)。得到了斜臭氧Z和UV-Bm透射率KtUV-B的月平均变化规律。对比了斜臭氧Z和UV-Bm透射率KtUV-B两个变量。对回归方程的斜率(β)、截距(α)和拟合线的标准误差(SE)进行了季节性统计。最小斜率出现在冬季,表明高倾斜臭氧Z的EER减少百分比大于g。斜率(β)在年内的变化范围从冬季的最小值0.2867到夏季的最大值0.3253,在冷湿和热干月份也表现出最小值和最大值。给出了总小时平均日红斑与总小时平均日宽带太阳总辐照(EER/G)的百分率的时间变率。UV-Best太阳辐射估计值与UV-Bm太阳辐射实测值吻合较好。太阳UV-B辐射的估计值与实测值的差值在3.1至4.25%之间。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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