大气中的水汽对太阳紫外辐射消光的可能机制分析

本文给出了北京地区晴天和实际天气条件下到达地面太阳紫外总辐射的一种计算方法，分析了影响到达地面太阳紫外总辐射的各主要因子的主次贡献，重点讨论了水汽在参与大气中的光化学反应过程中，对到达地面的太阳紫外总辐射消光的可能机制。     

南极长城站和中山站辐射特征的研究

对南极长城站和中山站1993～1994年辐射资料的分析表明:两站辐射分量的季节变化特征基本相似。但由于气候状况的差异,长城站到达地面的总辐射和吸收辐射分别为中山站的51%和42%。极昼期间（11～1月）中山站总辐射和紫外辐射总量均超过了青藏高原夏季（6～8月）的总量,两站净辐射夏半年为正,冬半年为负,显示出南极绿洲的辐射气候特点。     

宁波市紫外辐射分布特征及强度预报服务技术研究

利用2010—2015年宁波市紫外辐射强度资料、常规气象观测资料以及大气环境资料,分析宁波市紫外辐射强度的日、月、季节、年际变化规律及其与气象和环境条件的相关性,并对到达地表的紫外辐射与大气上界的太阳总辐射的比值η'进行逐步回归,建立η'的预报方程,最后利用辐射传输公式计算出到达地面的紫外辐射强度。预报方程充分考虑了太阳高度角,以及温度、降水、水汽、能见度等气象要素对紫外辐射的影响。并将统计方法与本地气候特征相结合,增加了气候特征判据。经检验,预报紫外线等级正确率为53. 2%,相差1级的占34. 5%,优于主观预报,能够提高现有的紫外线等级预报准确率。最后,提出一种适合本地的紫外线等级划分标准,并根据冬半年和夏半年分别制定相应的防御建议。     

东疆黑戈壁太阳紫外辐射变化特征

利用东疆红柳河黑戈壁下垫面陆气相互作用观测站2017年太阳紫外辐射、总辐射和气象站天气现象观测数据,对东疆黑戈壁不同时间尺度和不同天气背景下的太阳A波段紫外辐射(UVA)和B波段(UVB)的变化特征进行了分析。结果表明:紫外辐射UVA和UVB日变化呈正态分布,UVA、UVB最大瞬时辐照度为67.97、2.15 W·m^-2,最大曝辐量为2.09、0.05 MJ·m^-2,年曝辐量为400.31、8.63 MJ·m^-2;季节变化呈现夏季高、冬季低、春季高于秋季的特点;年变化呈现倒"U"型,年变化幅度呈夏季大、冬季小的趋势。紫外辐射占总辐射的比例呈夏高冬低的特点。不同天气下,其比例变化幅度也不相同,晴天大于雨天。太阳紫外辐射的月和年平均量以及紫外辐射年均值占总辐射年均值的比例,东疆黑戈壁地区都明显高于其他地区。     

影响上海地区太阳紫外辐射的研究

上海于1997年8月起建立了太阳紫外辐射强度观测点。分析了1998年8月－1999年7月用埃帕莱紫外辐射仪（Eppley Ultra-Violet Radiometer）所采集的到达地面太阳紫外辐射数据。研究了紫外辐射与影响它变化的各个因子之间的互相影响程度。     

1979～1996年期间北京地区太阳紫外总辐射的变化趋势

对实际天气条件下北京地区1990年1月至1992年8月太阳辐射观测资料进行了详细的分析,得到了实际天气条件下到达地面的太阳紫外总辐射的计算公式。结果表明,计算值与观测值吻合得比较好。最后,利用此公式计算了北京地区1979年1月～1996年6月的太阳紫外总辐射,并讨论了1979～1996年北京地区太阳紫外总辐射的变化趋势。     

南京地区紫外辐射初步研究

采用简化型辐射传播模型计算了南京地区到达地表的太阳紫外辐射（ＵＶ辐射）,同时根据地面紫外辐射的观测资料分析了南京地区紫外辐射的年变化、晴天与阴天的变化规律及与太阳总辐射的关系。     

基于卫星遥感的新疆地表太阳总辐射估算

为了实现地表太阳总辐射合理的精细化模拟,本文尝试将天文辐射分布式理论模型和总辐射气候学经验模型相结合,引入重采样后的FY-2G卫星遥感总云量资料,建立了基于卫星遥感数据的地表太阳总辐射估算模型,并以气象站点稀疏的新疆为例,完成年、季地表太阳总辐射的精细化空间模拟,同时对模拟结果进行分析和检验。结果表明:(1)新疆区域年天文辐射量由南向北递减,大致以天山为界,天山以南区域的年天文辐射量高于10 000 MJ·m^-2,天山以北低于9750 MJ·m^-2,三大山脉对天文辐射的影响非常明显;(2)基于条带状重采样后的FY-2G总云量建立的日照百分率模型,其模拟的新疆区域平均绝对误差14.4%,且空间分布更加客观;(3)新疆"单站单月式"地表太阳总辐射气候学估算模型中,相关系数在夏半年较高,冬半年略有下降,且a、b系数的互补关系较为稳定;(4)从地表太阳总辐射检验结果来看,全区地表太阳总辐射的均方根误差年平均3.08 MJ·m^-2,模拟结果夏半年好于冬半年,南疆好于北疆,其中乌鲁木齐误差最大;(5)新疆年地表太阳总辐射整体表现为由西北向东南逐渐增加的空间分布,南疆盆地的总辐射量高于北疆盆地,天山山区西部为低值中心,而春、夏季总辐射由西向东呈经向分布,秋、冬季则呈纬向分布。     

东疆黑戈壁太阳紫外辐射变化特征

本文利用东疆红柳河黑戈壁下垫面陆气相互作用观测站2017年太阳紫外辐射、总辐射和气象站天气现象观测数据，对东疆黑戈壁不同时间尺度和不同天气背景下的太阳紫外辐射A波段(UVA)和B波段（UVB）的变化特征进行了分析。结果表明：1）紫外辐射UVA和UVB日变化呈正态分布，UVA、UVB最大瞬时辐照度为67.97W·m-2、2.15W·m-2，日均最大曝辐量为2.09MJ·m-2和0.05MJ·m-2，年曝辐量为400.31 MJ·m-2和8.63 MJ·m-2；季节变化呈现夏季高，冬季低、春季高于秋季的特点；年变化呈现倒“U”型，年变化幅度呈夏季大，冬季小的趋势。2）紫外辐射占总辐射的比例呈夏高冬低的特点。不同天气下，其比例变化幅度也不相同，晴天大于雨天。3）太阳紫外辐射的月和年平均量以及紫外辐射年均值占总辐射年均值的比例，东疆黑戈壁地区都明显高于其他地区。     

影响太阳总辐射各主要因子的分析

本文通过分析北京地区１９９０年１－１２月晴天与实际天气条件下的太阳辐射和常规气象观测资料，得到了描述晴天和实际天气条件下的太阳总辐射的一种关系式，并着重分析了影响到达地面的太阳总辐射各因子的主次作用。     

山东禹城紫外辐射变化特征及其估测方程的建立

本文对2005～2011年山东禹城地区观测得到的紫外辐射的时间变化特征及紫外辐射与总辐射比值的变化特征进行了分析, 并结合气温、降水和露点温度资料建立了禹城地区的紫外辐射估测方程。结果表明:紫外辐射日累计值的变化范围为0.10～1.20 MJ m-2 d-1, 年平均值为0.468 MJ m-2 d-1;紫外辐射日、季节变化规律与总辐射一致, 季节变化都表现为冬季小夏季大, 最小值出现在1月, 最大值出现在6月, 日变化则呈现早晚小中午大的特征;紫外辐射与总辐射的比值范围为0.023～0.046, 其季节变化特征也是冬季小夏季大, 该比值随晴空指数的增大而减小, 而在晴空指数大于0.5时比较稳定。利用温度日较差(日最高气温与最低气温的差值)建立了紫外辐射估测方程, 决定系数R2达0.80, 平均相对误差为0.19, 估测紫外线等级与实测紫外线等级相差不大于1的数据占95%, 该方法可以较好地进行紫外辐射等级的估测。     

Precise estimation of hourly global solar radiation for micrometeorological analysis by using data classification and hourly sunshine

We have developed a method for estimating hourly global solar radiation (GSR) from hourly sunshine duration data. This procedure requires only hourly sunshine duration as the input data and utilizes hourly precipitation and daily snow cover as auxiliary data to classify time intervals into six cases according to weather conditions. To obtain hourly GSR using a simple algebraic form, a quadratic function of the solar elevation angle and the sunshine duration ratio is used. Daily GSR is given by a sum of hourly GSRs. We evaluated the performance of the newly developed method using data obtained at 67 meteorological stations and found that the estimated GSR is highly consistent with that observed. Hourly and daily root-mean-square misfits are approximately 0.2 MJ/m²/h (~55 W/m²) and 1.4 to 1.5 MJ/m²/day (~16 to 17 W/m²), respectively. Our classification of weather conditions is effective for reducing estimation errors, especially under cloudy skies. Since the sunshine duration is observed at more meteorological stations than GSR, the proposed new method is a powerful tool for obtaining solar radiation with hourly resolution and a dense geographical distribution. One of the proposed methods, GSRgrn, can be applicable to hourly GSR estimations at different observation sites by setting local parameters (the precipitable water, surface albedo, and atmospheric turbidity) suitable to the sites. The hourly GSR can be applied for various micrometeorological studies, such as the heat budget of crop fields.     

Estimation and Long-term Trend Analysis of Surface Solar Radiation in Antarctica: A Case Study of Zhongshan Station

Long-term,ground-based daily global solar radiation (DGSR) at Zhongshan Station in Antarctica can quantitatively reveal the basic characteristics of Earth’s surface radiation balance and validate satellite data for the Antarctic region.The fixed station was established in 1989,and conventional radiation observations started much later in 2008.In this study,a random forest (RF) model for estimating DGSR is developed using ground meteorological observation data,and a highprecision,long-term DGSR dataset is constructed.Then,the trend of DGSR from 1990 to 2019 at Zhongshan Station,Antarctica is analyzed.The RF model,which performs better than other models,shows a desirable performance of DGSR hindcast estimation with an R~2 of 0.984,root-mean-square error of 1.377 MJ m~(-2),and mean absolute error of 0.828 MJ m~(-2).The trend of DGSR annual anomalies increases during 1990–2004 and then begins to decrease after 2004.Note that the maximum value of annual anomalies occurs during approximately 2004/05 and is mainly related to the days with precipitation (especially those related to good weather during the polar day period) at this station.In addition to clouds and water vapor,bad weather conditions (such as snowfall,which can result in low visibility and then decreased sunshine duration and solar radiation) are the other major factors affecting solar radiation at this station.The high-precision,longterm estimated DGSR dataset enables further study and understanding of the role of Antarctica in global climate change and the interactions between snow,ice,and atmosphere.     

Characteristics of UV radiation at Tazhong of the Tarim Basin,west China

Tazhong station, located at the hinterland of the Taklimakan Desert in northwest China, experiences frequent dusty weather events during spring and summer seasons (its dusty season) caused by unstable stratified atmosphere, abundant sand source and strong low-level wind. On average, it has 246.2 dusty days each year, of which 16.2 days are classified as sand and dust storm days. To better understand the characteristic of solar ultraviolet (UV) radiation and factors influencing its variations under such an extreme environment, UV radiation data were collected continuously from 2007 to 2011 at Tazhong station using UVS-AB-T radiometer by Kipp and Zonen. This study documents observational characteristics of the UV radiation variations observed during the five-year period. Monthly UV radiation in this region varied in the range of 14.1–37.8 MJ m^?2 and the average annual amount was 320.7 MJ m^?2. The highest value of UV radiation occurred in June (62.5 W m^?2) while the lowest one in December (29.3 W m^?2). It showed a notable diurnal cycle, with peak value at 12:00–13:00 LST. Furthermore, its seasonal variation exhibited some unique features, with averaged UV magnitude showing an order of summer > spring > autumn > winter. The seasonal values were 37.0, 29.1, 24.9 and 15.9 MJ m^?2, respectively. In autumn and winter, its daily variations were relatively weak. However, significant daily variations were observed during spring and summer associated with frequent dust weather events occurring in the region. Further analysis showed that there was a significant correlation between the UV radiation and solar zenith angle under different weather conditions. Under the same solar zenith angle, UV radiation was higher during clear days while it was lower in sand and dust storm days. Our observations showed that there was a negative correlation between UV radiation and ozone, but such a relationship became absent in dusty days. The UV radiation was reduced by 6 % when cloud amount was 1–4 oktas, by 12 % when the cloud amount was 5–7 oktas, and by 24 % when the cloud amount was greater than 8 oktas. The relative reduction of UV radiation reached 26, 38, and 45 % in dust day, blowing sand day and sand and dust storm day, respectively. The results revealed that decrease in UV radiation can be attributed to cloud coverage and dust aerosols. Moreover, the reduction of UV radiation caused by dust aerosols was about 2–4 times greater than that caused by cloud coverage. These observational results are of value for improving our understanding of processes controlling UV radiation over sand desert and developing methods for its estimation and prediction.     

Relationship between Net Radiation and Broadband Solar Radiation in the Tibetan Plateau

The characteristics of net radiation (R_n)(0.3--10 μm) in Lhasa and Haibei in the Tibetan Plateau were analyzed based on long-term in-situ measurements of surface radiation data. The monthly average of daily R_n reached a minimum during the winter period followed by an increase until May and then a decline until January. This variation is consistent with solar activity. The annual mean daily total R_n values were 0.92 MJ m^-2 d^-1 and 0.66 MJ m^-2d^-1 in Lhasa and Haibei, respectively. A relationship between R_n and broadband solar radiation (R_s) was demonstrated by a good linear correlation at the two sites. R_n can be an accurate estimate from R_s. The estimated R_n values were similar to the observed values, and the relative deviations between the estimates and measurements of R_n were 2.8% and 3.8% in Lhasa and Haibei, respectively. The application of the R_n estimating model to other locations showed that it could provide acceptable estimated R_n values from the R_s data. Furthermore, we analyzed the influence of clouds on R_n by different clear index (K_s), defined as the ratio of R_s to the extraterrestrial solar irradiance on a horizontal surface. The results indicate that more accurate results are associated with increased cloudy conditions. The influence of the albedo was also considered, but its inclusion in the model resulted in only a slight improvement. Because surface albedo is not usually measured, an expression based solely on global solar radiation could be of more extensive use.     

Influence of weather conditions and spatial variability on glacier surface melt in Chilean Patagonia

In order to clarify how differences in weather conditions affect the surface heat balance of a large maritime glacier, meteorological observations were carried out in the ablation area of Glaciar Exploradores in the Chilean Patagonia during the austral summer of 2006/2007. Under cloudy/rainy weather, when the air temperature and wind speed were high due to advection, the average melting heat was 18.8 MJ m^?2 day^?1 and the turbulent heat fluxes contributed 35% of the total melt. During clear weather, the average melting heat was 16.9 MJ m^?2 day^?1 and 13% of the total was the turbulent heat fluxes. A decrease in air temperature due to the development of the glacier boundary layer on clear days will lead to an overestimation of the melt using the air temperature at a weather station outside of the glacier.     

2011年2月—2012年1月东南极高原辐射平衡观测研究

利用东南极高原熊猫-1自动气象站2011年2月—2012年1月观测的辐射资料和相关资料,对辐射分量和辐射平衡的季节变化进行了研究。结果表明,夏季是东南极高原获得太阳能的主要时段,总辐射通量夏季平均为365.0 W/m²,总量达到2752.1 MJ/m²,占全年总辐射量的58%。各个季节均能出现总辐射瞬时值大于大气顶水平总辐射,春季发生频率最高,冬季最小,总辐射平均日变化呈单峰型。大气长波辐射除夏季外,日变化不明显。冰雪面长波辐射除冬季外,各季节平均日变化呈明显的单峰单谷型。净辐射12月和1月为很小的正值,其他月份为负值。年平均净辐射为 -8.7 W/m²,表明地表相对于大气为冷源。该站的辐射平衡特征与其他南极内陆高原站相似,雪面具有强烈的辐射冷却效应,导致净辐射绝对值都小于下降风区。     

Parameterization and mapping of solar radiation in data sparse regions

Knowledge of temporal and spatial variation of solar radiation is essential for many applications. In this work, a simple and feasible procedure is conducted to map the daily solar radiation for Liaoning province, one of the most important agricultural areas in China, but with sparsely measured solar radiation data. The daily sunshine duration are interpolated to the whole area, subsequently, solar radiation are calculated by ?ngstr?m-Prescott model, the generic parameters of which are determined by least square to minimize the overall fitting residual between the ratio of actual to potential sunshine duration and the ratio of actual to extra-terrestrial solar radiation of the sites where solar radiation are available. In other local regions with sparse data, mapping of the solar radiation could be done following the simple procedure. In the present study area, using the interpolated daily sunshine duration data by ANUSPLIN, ?ngstr?m-Prescott model with the generic parameters (a = 0.505, and b = 0.204) returns reasonable results, with the overall RMSE of 2.255 MJ m^?2, and RRMSE of 16.54%. The daily solar radiation varies between 5.26 in December and 22.74 MJ m^?2 in May, and shows an obviously spatial variation which is mainly contributed to the climate and topography. The substitution of solar radiation from nearby station is preferred to estimation by ?ngstr?m-Prescott model if the distance between the stations falls below the threshold of 135 ± 15 km. The RMSE of such substitution increases by approximately 0.157 MJ m^?2 per 10 km.     

五道梁地区的太阳紫外辐射

该文利用１９９３年９月－１９９４年８月五道梁站的太阳辐射观测资料。分析了该地区太阳紫外辐射的气候学特征。结果表明：该地区的太阳紫外辐射年平均日总量为０．７３ＭＪ／ｍ＾２，小于拉萨地区、而大于高原东北侧的河南走廊地区；紫外辐射的瞬时极大值较大，７月份可达５６Ｗ／ｍ＾２，大于河区而略小于拉萨地区。     

Analysis of solar radiation on the surface estimated from GWNU solar radiation model with temporal resolution of satellite cloud fraction

Preliminary analysis with a solar radiation model is generally performed for photovoltaic power generation projects. Therefore, model accuracy is extremely important. The temporal and spatial resolutions used in previous studies of the Korean Peninsula were 1 km × 1 km and 1-h, respectively. However, calculating surface solar radiation at 1-h intervals does not ensure the accuracy of the geographical effects, and this parameter changes owing to atmospheric elements (clouds, aerosol, ozone, etc.). Thus, a change in temporal resolution is required. In this study, one-year (2013) analysis was conducted using Chollian geostationary meteorological satellite data from observations recorded at 15-min intervals. Observation data from the intensive solar site at Gangneung-Wonju National University (GWNU) showed that the coefficient of determination (R²), which was estimated for each month and season, increased, whereas the standard error (SE) decreased when estimated in 15-min intervals over those obtained in 1-h intervals in 2013. When compared with observational data from 22 solar sites of the Korean Meteorological Administration (KMA), R² was 0.9 or higher on average, and over- or under-simulated sites did not exceed 3 sites. The model and 22 solar sites showed similar values of annual accumulated solar irradiation, and their annual mean was similar at 4,998 MJ m^?2 (3.87 kWh m^?2). These results show a difference of approximately ± 70 MJ m^?2 (± 0.05 kWh m^?2) from the distribution of the Korean Peninsula estimated in 1-h intervals and a higher correlation at higher temporal resolution.