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南极 Dome C 地区全球太阳辐射长期变化及其潜在影响。

Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica).

机构信息

LAGEO, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029, China.

European Commission, Joint Research Centre, Via Fermi 2749, 21027 Ispra, Italy.

出版信息

Int J Environ Res Public Health. 2022 Mar 6;19(5):3084. doi: 10.3390/ijerph19053084.

Abstract

An empirical model to predict hourly global solar irradiance under all-sky conditions as a function of absorbing and scattering factors has been applied at the Dome C station in the Antarctic, using measured solar radiation and meteorological variables. The calculated hourly global solar irradiance agrees well with measurements at the ground in 2008-2011 (the model development period) and at the top of the atmosphere (TOA). This model is applied to compute global solar irradiance at the ground and its extinction in the atmosphere caused by absorbing and scattering substances during the 2006-2016 period. A sensitivity study shows that the responses of global solar irradiance to changes in water vapor and scattering factors (expressed by water vapor pressure and S/G, respectively; S and G are diffuse and global solar irradiance, respectively) are nonlinear and negative, and that global solar irradiance is more sensitive to changes in scattering than to changes in water vapor. Applying this empirical model, the albedos at the TOA and the surface in 2006-2016 are estimated and found to agree with the satellite-based retrievals. During 2006-2016, the annual mean observed and estimated global solar exposures decreased by 0.05% and 0.09%, respectively, and the diffuse exposure increased by 0.68% per year, associated with the yearly increase of the S/G ratio by 0.57% and the water vapor pressure by 1.46%. The annual mean air temperature increased by about 1.80 °C over the ten years, and agrees with the warming trends for all of Antarctica. The annual averages were 316.49 Wm for the calculated global solar radiation, 0.332 for S/G, -46.23 °C for the air temperature and 0.10 hPa for the water vapor pressure. The annual mean losses of solar exposure due to absorbing and scattering substances and the total loss were 4.02, 0.19 and 4.21 MJ m, respectively. The annual mean absorbing loss was much larger than the scattering loss; their contributions to the total loss were 95.49% and 4.51%, respectively, indicating that absorbing substances are dominant and play essential roles. The annual absorbing, scattering and total losses increased by 0.01%, 0.39% and 0.28% per year, respectively. The estimated and satellite-retrieved annual albedos increased at the surface. The mechanisms of air-temperature change at two pole sites, as well as a mid-latitude site, are discussed.

摘要

已经应用了一种经验模型来预测在所有天空条件下的小时全球太阳辐照度,该模型是作为吸收和散射因子的函数,在南极的 Dome C 站进行了测量。在 2008-2011 年(模型开发期间)和在大气顶部(TOA),用测量的太阳辐射和气象变量计算出的小时全球太阳辐照度与地面测量结果吻合较好。该模型用于计算 2006-2016 年期间地面的全球太阳辐照度及其被吸收和散射物质在大气中的衰减。敏感性研究表明,全球太阳辐照度对水汽和散射因子(分别用水汽压力和 S/G 表示,S 和 G 分别是漫射和全球太阳辐照度)变化的响应是非线性和负的,并且全球太阳辐照度对散射的变化比水汽更敏感。应用该经验模型,估计了 2006-2016 年 TOA 和表面的反照率,发现与基于卫星的反演结果相符。在 2006-2016 年期间,观测到的和估计的全球太阳辐照度的年平均值分别减少了 0.05%和 0.09%,而漫射辐照度每年增加 0.68%,这与 S/G 比值每年增加 0.57%和水汽压力增加 1.46%有关。在过去十年中,年平均气温上升了约 1.80°C,与南极洲所有地区的变暖趋势一致。计算出的全球太阳辐射的年平均值为 316.49 Wm,S/G 为 0.332,空气温度为-46.23°C,水汽压力为 0.10 hPa。由于吸收和散射物质导致的太阳辐照度年平均损失和总损失分别为 4.02、0.19 和 4.21 MJ m。年平均吸收损失远大于散射损失;它们对总损失的贡献分别为 95.49%和 4.51%,表明吸收物质是主要的,起着至关重要的作用。吸收、散射和总损失的年增长率分别为 0.01%、0.39%和 0.28%。估计的和卫星反演的年度反照率在地面增加。讨论了两极站点以及中纬度站点的空气温度变化机制。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1db9/8910517/f84224dbc4fd/ijerph-19-03084-g001.jpg

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