Measurements on Solar Energy Resources in the Mt. Everest Region

Norsang Gelsor, L. Juan, Tsoja Wangmo, Lagba Tunzhup, Nuozhen Gelsor
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引用次数: 1

Abstract

Research on solar radiation in the Mt. Everest region provides great interests for the strategies of solar energy utilization, climate change and environmental sustainability etc. We present measurement results of global horizontal irradiance, solar spectral irradiance and solar UV irradiance performed with the Dutch CMP11 Pyranometers, the German RAMSES Hyperspectral Irradiance Sensors and the Norwegian NILU-UV Irradiance Meters respectively in the Mt. Everest region during 2008 to 2017. The results show that the solar energy resources are extremely rich in that area, the daily maximum of global horizontal irradiance levels are even frequently exceed the solar constant value of 1368W/m2 during monsoon season, from May to August in that region. The highest daily maximum value reached 1500 W/m2 occurred on July 13, 2017. The annual average of the daily global horizontal irradiance is about 18.4 MJ/m2/d, the daily global horizontal irradiance varies from 13.8 to 23.9 MJ/m2/d, indicates that there are abundant solar energy in that alpine zone. The instruments record that even during the winter time (October to January) more than 15 days of each month are absolute clear days, it shows 28 clear days in November of 2016. It points out that more solar energy can be existed during the winter time due to dry season. The solar spectral irradiance was performed for the first time in this special environment presenting the characteristics of solar spectrum over the region. It reveals not only how abundant the spectral irradiance is, but also rich information about the atmospheric composition over the sky. It is well known that the solar UV radiation strongly impacts on the ecological environment and human health. The measurement results of solar UV dose rates as well as their impact factors (ozone and cloud) during the period of 2008 to 2017 are also presented. Satellite data are also used to see how the solar irradiance is distributed over the Himalayan region in summer, including Mt. Everest.
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珠穆朗玛峰地区太阳能资源的测量
珠穆朗玛峰地区太阳辐射的研究对太阳能利用策略、气候变化和环境可持续性等具有重要意义。本文介绍了2008年至2017年在珠穆朗玛峰地区分别使用荷兰CMP11强辐射计、德国RAMSES高光谱辐照度传感器和挪威NILU-UV辐照度计进行的全球水平辐照度、太阳光谱辐照度和太阳紫外线辐照度的测量结果。结果表明,该地区太阳能资源极为丰富,5 ~ 8月季风季节全球水平辐照水平日最大值甚至经常超过太阳常数1368W/m2。日最大值在2017年7月13日达到1500 W/m2。全球日水平辐照度的年平均值约为18.4 MJ/m2/d,全球日水平辐照度在13.8 ~ 23.9 MJ/m2/d之间变化,表明该高寒地区太阳能资源丰富。仪器记录,即使在冬季(10月至1月),每个月也有超过15天是绝对晴天,2016年11月有28天是绝对晴天。指出由于干旱季节,冬季可以利用更多的太阳能。首次在这一特殊环境下进行了太阳光谱辐照度的实测,反映了该区域太阳光谱的特征。它不仅揭示了光谱辐照度的丰富程度,而且还提供了有关天空大气成分的丰富信息。众所周知,太阳紫外线辐射对生态环境和人体健康的影响很大。介绍了2008 - 2017年太阳紫外线剂量率及其影响因子(臭氧和云)的测量结果。卫星数据也被用来观察夏季太阳辐照度在喜马拉雅地区的分布,包括珠穆朗玛峰。
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