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DOI | 10.3390/en16207093 |
Calibrating the Ångström-Prescott Model with Solar Radiation Data Collected over Long and Short Periods of Time over the Tibetan Plateau | |
Liu, Jiandong; Shen, Yanbo; Zhou, Guangsheng; Liu, De-Li; Yu, Qiang; Du, Jun | |
发表日期 | 2023 |
EISSN | 1996-1073 |
卷号 | 16期号:20 |
英文摘要 | As the coefficients of the angstrom ngstrom-Prescott model is site-dependent, the sparsity of radiation stations in regions like the Tibetan Plateau (TP) presents challenges for model calibration. Due to the unique climate and the clean air conditions over the TP, it might be feasible to calibrate the angstrom ngstrom-Prescott model with short-term observations from scientific expeditions. To test this hypothesis, we used various datasets with different lengths at four stations, together with 435 daily radiations measured during a scientific expedition at Banga in the central TP from 2014 to 2015, to calibrate the angstrom ngstrom-Prescott model. We found that calibration with a 1-year data length resulted in model performances comparable to those with a 20-year data length. Analysis of the expedition observations showed that the monthly average daily radiation ranged from 15.2 MJ/m(2)d in December 2014 to 26.5 MJ/m(2)d in July 2015, with an average value of 20.6 MJ/m(2)d. When this set of expedition data was used for calibration, the angstrom ngstrom-Prescott model performed well with an NSE (Nash-Sutcliffe efficiency) of 0.820. If no data were available for calibration, the coefficients of the angstrom ngstrom-Prescott model could also be directly calculated by parameterization methods established with calibrations at the other radiation stations. In this situation, the LiuJD method performed the best with the highest NSE of 0.792, followed by the LiuXY method with an NSE of 0.764. The FAO method performed poorly with an NSE of 0.578, while the Gopinathan method performed the worst with the lowest NSE of 0.218. Thus, the best strategy to calibrate the angstrom ngstrom-Prescott model in the Tibetan Plateau is to use data from local observations, even if collected over short periods. When these are not available, the coefficients of the angstrom ngstrom-Prescott model should be calculated using the parameterization method established with calibrations over the Tibetan Plateau. |
关键词 | solar radiationangstrom ngstrom-Prescott modelTibetan Plateauscientific expedition |
英文关键词 | SUNSHINE DURATION; METEOROLOGICAL DATA; GLOBAL RADIATION; TEMPERATURE; PREDICTION; FORMULA |
WOS研究方向 | Energy & Fuels |
WOS记录号 | WOS:001092649100001 |
来源期刊 | ENERGIES |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/283851 |
作者单位 | China Meteorological Administration; Chinese Academy of Meteorological Sciences (CAMS); China Meteorological Administration; NSW Department of Primary Industries; Northwest A&F University - China |
推荐引用方式 GB/T 7714 | Liu, Jiandong,Shen, Yanbo,Zhou, Guangsheng,et al. Calibrating the Ångström-Prescott Model with Solar Radiation Data Collected over Long and Short Periods of Time over the Tibetan Plateau[J],2023,16(20). |
APA | Liu, Jiandong,Shen, Yanbo,Zhou, Guangsheng,Liu, De-Li,Yu, Qiang,&Du, Jun.(2023).Calibrating the Ångström-Prescott Model with Solar Radiation Data Collected over Long and Short Periods of Time over the Tibetan Plateau.ENERGIES,16(20). |
MLA | Liu, Jiandong,et al."Calibrating the Ångström-Prescott Model with Solar Radiation Data Collected over Long and Short Periods of Time over the Tibetan Plateau".ENERGIES 16.20(2023). |
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