短波辐射参数化方案对WRF-Solar预测不同气候带全球水平辐照度的影响:以印度为例

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Naveen Krishnan , K. Ravi Kumar
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引用次数: 0

摘要

像印度这样的发展中国家有一个雄心勃勃的目标,即在未来扩大其太阳能系统,用于发电和过程热应用。因此,对于像印度这样的发展中国家来说,拥有一种可靠的技术来预测未来的短波辐射,以有效地管理需求和供应是必不可少的。本研究使用天气研究预报-太阳(WRF-Solar)预测未来14天的全球水平辐照度(GHI),并使用Solcast®数据验证结果。对Dudhia、Goddard流体动力学实验室(GFDL)、New Goddard和大气环流模式中的快速辐射传输模式(RRTMG)等4种短波参数化方案在印度暖气区和暖气区等不同气候区域进行了试验。潮湿、炎热;以找出提高GHI预测精度的最佳配置。并对一年中的不同季节进行了参数化方案的敏感性分析。在温暖中;在湿润气候带,Dudhia方案的均方根误差(RMSE)最小,为133.67 W/m2,其次是New Goddard、RRTMG和GDFL方案,均方根误差分别增加了6.67%、7.07%和7.61%。在复合气候带,RRTMG方案的平均RMSE低于其他3种方案,平均RMSE为134.58 W/m2,其次是Dudhia、New Goddard和GFDL,平均RMSE分别提高了3.02%、4.18%和12.02%。在干热气候带,Dudhia方案的平均RMSE低于其他3个方案,平均RMSE为133.20 W/m2,其次是GFDL、RRTMG和New Goddard方案,平均RMSE分别提高了0.61%、4.10%和5.71%。尽管气候条件恶劣,但由于夏季天气晴朗,所有计划的表现都较好,而在季风季节,由于阴天的情况,所有计划的表现都低于平均水平。研究结果更有利于太阳能发电的利益相关者和电网运营商在并网和供需管理中高效运行。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Impact of shortwave radiation parameterization schemes in predicting global horizontal irradiance for various climatic zones by WRF-Solar: A case study in India
A developing country like India has an ambitious target of expanding their solar energy systems in the future for generating power and process heat applications. Hence, it is integral for a developing country such as India to have a robust technique to predict the shortwave radiation in the future to effectively manage the demand and supply. Weather Research Forecasting - Solar (WRF-Solar) is employed in this study to predict the Global Horizontal Irradiance (GHI) for 14 days ahead and results are validated with the Solcast® data. Four shortwave parameterization schemes such as Dudhia, Goddard Fluid Dynamics Laboratory (GFDL), New Goddard, and Rapid Radiative Transfer Model in General Circulation Model (RRTMG) have been tested for various climatic regions in India such as warm & humid, hot & dry and composite to find out the optimal configuration that improves the accuracy of GHI prediction. It has also been performed for different seasons in a year to conduct the sensitivity analysis of the parameterization schemes. In the warm & humid climatic zone, the Dudhia scheme outperformed the other three schemes by yielding less mean Root Mean Square Error (RMSE) of 133.67 W/m2, then followed by New Goddard, RRTMG and GDFL with increased mean RMSE of 6.67 %, 7.07 %, and 7.61 % respectively. In Composite climatic zone, the RRTMG scheme performed better than the other three schemes by yielding less mean RMSE of 134.58 W/m2, then followed by Dudhia, New Goddard and GFDL with increased mean RMSE of 3.02 %, 4.18 %, and 12.02 % respectively. For hot and dry climatic zone, the Dudhia scheme performed better than the other three schemes by yielding less mean RMSE of 133.20 W/m2, then followed by GFDL, RRTMG and New Goddard with an increased mean RMSE of 0.61 %, 4.10 %, and 5.71 % respectively. Despite the climatic conditions, all the schemes performed better in the summer season due to clear skies and below average in the monsoon season due to overcast conditions. The findings of the research are more beneficial to the stakeholders indulged in power generation using solar energy and grid operators for efficient operation in grid integration along with the management of demand and supply.
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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