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1.
Summary In this paper, we analyze global, direct and diffuse solar radiation data on a horizontal surface observed at stations in Shanghai, Nanjing and Hangzhou for the period of 1961 to 2000. The data include monthly averages of the daily clearness index (G/G0: the ratio of global to extraterrestrial solar radiation) and the diffuse fraction (D/G: the ratio of diffuse to global solar radiation. The present study has processed and analyzed the data, including variables or statistics of mean, and annual monthly and daily total, the diurnal variation and the frequency of daily totals of global solar radiation. A correlation between daily values of clearness index and diffuse fraction is obtained and recommended correlation equations were calculated. The annual variations and trend of yearly series are analyzed for daily global, direct and diffuse radiation on a horizontal surface, as well as for daily clearness index and diffuse fraction in Shanghai, Nanjing and Hangzhou. The results show: 1) the east China is characterized by a decrease in global and direct radiation and a little increase in diffuse radiation and a negative linear relationship was obtained between clearness index and diffuse fraction. 2) The annual variations of global, direct and diffuse radiation for Shanghai, Nanjing and Hangzhou are similar with relative low values of global and direct radiation in June due to the Meiyu period. 3) The acceleration of air pollution and decrease of relative sunshine are the possible causes for the decrease of global and direct radiation.  相似文献   

2.
敦煌地区荒漠戈壁地表热量和辐射平衡特征的研究   总被引:83,自引:4,他引:79  
张强  曹晓彦 《大气科学》2003,27(2):245-254
利用2000年5月25日~6月17日"敦煌试验"在戈壁的微气象观测资料,分析了极端干旱地区晴天、阴天和降水等天气条件下的地表辐射平衡、热量平衡和土壤温度等微气象特征的日变化规律.发现在不同天气条件微气象特征有很大变化.但观测期间的平均微气象特征与晴天比较接近,天气过程的影响不是很大,平均的总辐射、净辐射和感热通量与晴天的比值在白天基本大于0.8.观测期间的平均Bowen比全天大于1,在白天都在10以上,最大超过100.  相似文献   

3.
北京城市紫外辐射变化特征及经验估算方程   总被引:10,自引:1,他引:10  
胡波  王跃思  刘广仁 《高原气象》2007,26(3):511-518
利用2004年4月—2005年6月在中国科学院大气物理研究所铁塔分部的紫外辐射观测数据,分析了北京城市紫外辐射的变化特征,结果表明,紫外辐射的变化规律与太阳总辐射一致,紫外辐射与总辐射的比值变化范围在0.02~0.04之间,晴天恒定在0.03,阴天在0.04左右,在沙尘暴过程中比值最小,为0.02。通过分析紫外辐射与大气质量数和平均晴空指数之间的关系,建立了适合于北京的全天候紫外辐射的估算方程。利用建立的估算方程及观测的总辐射值进行了紫外辐射的估算,紫外辐射的计算相对误差在10%以内。  相似文献   

4.
Daily global solar radiation is an important input required in most crop models. In the present study, a sunshine-based model, the ?ngstr?m–Prescott model, is employed to estimate daily global solar radiation on a horizontal surface during the growing season in Northeast China. Data from six control groups are used. The controls include the entire sequence, precipitation days, and non-precipitation days both during the growing season and year-round. Estimations are validated by comparing the calculated values with the corresponding measured values. The results indicate that estimating daily global solar radiation during the growing season using data only from the growing season is better than using year-round data. Classifying days with respect to precipitation and non-precipitation is also unnecessary. The performance on estimating daily global solar radiation during the growing season using the entire data in growing season performs best. A sunshine-based equation is obtained using our method to estimate growing season daily radiation for all meteorological stations in Northeast China. The approved approach is expected to be beneficial to crop models and other agricultural purposes.  相似文献   

5.
A method(Rieland,1985)has been modified to determine the downward solar radiation at ground overEast Asia,using GMS-3 data of the satellite with a spatial resolution of 10×10 krn~2 and a time interval of 3hours.The distributions of the monthly mean global radiation are obtained for January,April,July and Octoberof 1985.These results illustrate that the topography effect of the Tibetan Plateau is not negligible.The valuesof global radiation over the high Tibetan Plateau during all seasons are higher than those in the lower-levelsurroundings.By comparing model results with ground observed data, the relative errors in monthly averagesof global radiation are 2.8% for clear sky and 6.3%,5.3%,5.0% and 4.5% for cloudy sky in January,April,July and October,respectively.The relative error in daily global radiation during the snow-free season is lessthan 20% and larger than 20% in snow-covered winter.We,however,had no data for these comparisons whichwere measured directly at the Plateau during the year 1985.  相似文献   

6.
为研究我国不同地区住宅通过垂直墙面上的窗口实际接受到的太阳辐射量空间分布特征,以卡斯特洛夫公式为基础,建立了各朝向墙面晴天太阳总辐射和直接辐射小时总量的计算方案。使用水汽压和海拔高度拟合了公式中的参数,计算了我国各地满足国家标准对住宅间距要求下的水平面和垂直墙面辐射量,并绘制了分布图。研究发现:大寒日各朝向墙面晴天最大2 h辐射量空间分布受纬度和大气透明度共同影响,青藏高原为全国高值中心,川黔地区为低值中心。在我国东部地区,与水平面辐射量随纬度增加而降低的规律相反,同样是辐射量最大的2 h日照时间,纬度越高的地区南墙面接受的太阳辐射量就越大。与南墙相比,东、西墙面接收的最大2 h辐射量明显偏小,不能发挥阳光对健康和卫生的作用。上述结果表明,从大寒日建筑底层南墙面接收的最大2 h辐射量上看,适当放宽北方地区日照间距标准具有一定可行性。  相似文献   

7.
Analysis of solar radiation over Egypt   总被引:1,自引:0,他引:1  
Summary  The database utilized in this analysis consisted of daily sunshine duration and hourly global and diffuse radiation on a horizontal surface (for Matruh Cairo, and Aswan), and normal incidence beam radiation (for Cairo and Aswan only). Monthly-average hourly and daily values are reported for each of these three types of measured radiation, together with the calculated monthly-average daily values for the components of global radiation, horizontal beam and diffuse radiation. The monthly-average hourly and daily clearsky index values have also been calculated and analyzed. Monthly-average daily frequency distributions of the clearsky index values are reported for each month. The annual-average daily global irradiation values are 19.4, 18.67, and 21.78 MJ/m2 and for diffuse irradiation they are 6.34, 6.65 and 6.23 MJ/m2 for Matruh, Cairo and Aswan, respectively. For the normal incidence beam irradiation the annual-average daily values are 16.94 and 24.46 MJ/m2 for Cairo and Aswan, respectively. The annual-average daily fractions of the direct component of horizontal global radiation are 0.70, 0.61 and 0.72 for the three stations, respectively. The annual-average daily values for the clearsky index are 0.585, 0.566, and 0.648, and the average frequency of clear days annually are 67.3, 42.3 and 77.6% respectively. The annual variations and trend analysis were analyzed for daily global, direct, and diffuse radiation on a horizontal surface, daily sunshine duration, and for the daily ratios G/G0, and D/G for the stations Matruh, Cairo and Aswan. The distribution of these components of radiation and their ratios over the study stations in Egypt is also discussed. The results show that Egypt is characterized by relatively high average-daily radiation rates, both global and direct, and a relatively high frequency of clear days. Cairo, due to its urbanization and high pollution, has relatively low average-daily radiation rates, particularly in direct radiation, and the frequency of clear days. Received February 26, 1998 Revised February 4, 1999  相似文献   

8.
太阳能光伏发电已成为仅次于水电和风能的第三大可再生能源,光伏发电受云量时空变化的影响较大,因此准确模拟云天太阳辐射的时空变化对电网安全运行至关重要。围绕如何减小中尺度气象模式的云初始场误差,进而改进云天的太阳辐射模拟这一关键科学问题,本文通过研究基于卫星资料同化的LAPS(Local Analysis Prediction System)多时间层三维云分析同化方法,改进三维云结构,并将LAPS模式输出结果作为WRF(Weather Research and Forecasting)模式的初始场,模拟了2008年1月及夏季(6~8月)北京地区的总云量和总辐射的时空分布,重点分析了多云和有降水天气过程总辐射的模拟改进效果及其原因。结果表明,同化前后的总云量模拟值与观测值的时间变化趋势基本一致,但大部分时次总云量的模拟值低于观测值;大部分多云及降水时段同化后总云量模拟值较接近于实测值。1月晴天、多云天以及夏季晴天同化前后总辐射模拟值与实测值的时间变化趋势较一致,但同化前后两者的相关性差异不明显;晴天条件下同化前后总辐射模拟值均低于实测值,1月多云条件下多数时段同化后总辐射模拟误差减小不明显,与总云量的改进效果不显著有关。夏季多云、有降水及6月典型降水三种天气条件下同化前后总辐射模拟值与观测值的相关性稍差,同化后两者的相关性较同化前有所改进,尤其是6月典型降水过程改进效果较明显;同化前总辐射模拟误差较大,而同化后误差显著减小,尤其是6月典型降水过程同化后均方根误差和平均相对误差较同化前分别减小了102.6 W m-2和355.9%,最大相对误差减小更显著;同化后总辐射模拟误差小于同化前的比例高达75%,即大部分时刻同化后模拟误差小于同化前。多云和有降水天气过程总辐射模拟效果的显著改进与总云量的改进密切相关,即同化后总云量模拟值增加,云的反射和散射作用增强,导致模拟总辐射减小,即更接近于实测总辐射值。研究结果对于多云和降水天气条件下太阳辐射的模拟效果改进、太阳能资源客观评估以及光伏电站的发电量预测具有一定的科学和实际应用价值。  相似文献   

9.
Plants require solar radiation for photosynthesis and their growth is directly related to the amount received, assuming that other environmental parameters are not limiting. Therefore, precise estimation of photosynthetically active radiation (PAR) is necessary to enhance overall accuracies of plant growth models. This study aimed to explore the PAR radiant flux in the San Francisco Bay Area of northern California. During the growing season (March through August) for 2?years 2007?C2008, the on-site magnitudes of photosynthetic photon flux densities (PPFD) were investigated and then processed at both the hourly and daily time scales. Combined with global solar radiation (R S) and simulated extraterrestrial solar radiation, five PAR-related values were developed, i.e., flux density-based PAR (PPFD), energy-based PAR (PARE), from-flux-to-energy conversion efficiency (fFEC), and the fraction of PAR energy in the global solar radiation (fE), and a new developed indicator??lost PARE percentages (LPR)??when solar radiation penetrates from the extraterrestrial system to the ground. These PAR-related values indicated significant diurnal variation, high values occurring at midday, with the low values occurring in the morning and afternoon hours. During the entire experimental season, the overall mean hourly value of fFEC was found to be 2.17???mol?J?1, while the respective fE value was 0.49. The monthly averages of hourly fFEC and fE at the solar noon time ranged from 2.15 in March to 2.39???mol?J?1 in August and from 0.47 in March to 0.52 in July, respectively. However, the monthly average daily values were relatively constant, and they exhibited a weak seasonal variation, ranging from 2.02?mol?MJ?1 and 0.45 (March) to 2.19?mol?MJ?1 and 0.48 (June). The mean daily values of fFEC and fE at the solar noon were 2.16?mol?MJ?1 and 0.47 across the entire growing season, respectively. Both PPFD and the ever first reported LPR showed strong diurnal patterns. However, they had opposite trends. PPFD was high around noon, resulting in low values of LPR during the same time period. Both were found to be highly correlated with global solar radiation R S, solar elevation angle h, and the clearness index K t. Using the best subset selection of variables, two parametric models were developed for estimating PPFD and LPR, which can easily be applied in radiometric sites, by recording only global solar radiation measurements. These two models were found to be involved with the most commonly measured global solar radiation (R S) and two large-scale geometric parameters, i.e., extraterrestrial solar radiation and solar elevation. The models were therefore insensitive to local weather conditions such as temperature. In particular, with two test data sets collected in USA and Greece, it was verified that the models could be extended across different geographical areas, where they performed well. Therefore, these two hourly based models can be used to provide precise PAR-related values, such as those required for developing precise vegetation growth models.  相似文献   

10.
A simple model is developed which estimates daily global radiation at the floor of a non-homogeneous Eucalyptus forest. Model input parameters are easily derived from field measurements and consist of individual tree location, tree height, maximum canopy width and its corresponding height, height of the lowest branch and trunk thickness. In addition, the model requires values for global and diffuse irradiance in the open. The tree canopy is represented as a series of spheres containing leaves which are homogeneously spaced but are oriented in the vertical plane. This configuration closely approaches that of actual eucalyptus trees. A Monte-Carlo approach is used to estimate the albedo of the unit sphere as a function of solar zenith angle. At a given combination of solar zenith and azimuth angle, the model estimates the solar irradiance at a specific forest floor location.The model, when tested against pyranometer measurements, predicted daily solar irradiance with a correlation of 0.98 and a standard error of 0.98 MJ m-2 day-1. This good performance is attributed to the spatial averaging of the radiation fluxes over the entire day, and the relatively low sensitivity of the calculated solar irradiance to sphere albedo.  相似文献   

11.
Summary A statistical analysis and inter-comparison of the solar UVB, UVA and global radiation for Beer Sheva and Neve Zohar (Dead Sea) are presented utilizing data measured from January 1995 through December 2002. Beer Sheva is located approximately 65km to the west of and 700m above Neve Zohar. The monthly average hourly and daily values for all radiation types at both sites are reported. The standard errors of the monthly average daily values have been calculated in order to ascertain whether the average daily radiation intensities are representative, i.e. if the magnitude of the standard error is less than the inherent measurement uncertainty of the instruments, and, thereby, justify an inter-comparison between the two sites. The relative magnitude of the global, UVB and UVA radiation intensity at the two sites is attributed to the enhanced scattering of the incident solar radiation at the Dead Sea location due to the longer optical path length it must traverse to arrive at the Dead Sea, the lowest terrestrial point on earth. The degree of attenuation of solar radiation due to the scattering phenomena is inversely proportional to the wavelength raised to some power and, consequently, it is greatest for UVB and negligible for global radiation.  相似文献   

12.
吴其劻 《气象学报》1987,45(3):290-296
本文根据1983—1984年全国14个不同气候特点的日射站每日逐时照度与日射同步观测资料计算了总辐射光当量值,提出用纬度、海拔高度、地面平均绝对湿度和日照时数建立计算总辐射光当量的多元回归方程。用14个测站全年和各月平均总辐射光当量值检验所建立多元回归方程计算的相应总辐射光当量值表明,计算值的相对误差均小于10%。 我们用14个测站资料建立的计算总辐射光当量回归方程计算了全国464个测站的总辐射光当量值。总照度可由总辐射光当量与总辐射的乘积获得。根据各测站的总辐射光当量和总辐射值,便可计算出这些测站的光气候值,绘制我国光气候图。  相似文献   

13.
Ultraviolet (UV) solar radiation has a significant influence on human health, the environment and climate. A series of measurements, including UV radiation (290 400 nm) and global solar radiation (Rs), were continuously recorded from August 2004 at the Lhasa and Haibei sites on the Tibetan Plateau. Both observation sites' altitudes are above 3000 m and have similar meteorological conditions. The data from 2005 2006 was used to identify the varying characteristics of UV radiation. It's relation to the clearness index Ks, the relative optical mass mr, and Rs were established. The annual mean values of total daily UV radiation are 0.92 and 0.67 MJ m^-2 at Lhasa and Haibei, respectively. The UV radiation in Lhasa represented 4.6% of the global solar radiation while in Haibei this percentage was 4.2%. In the case of clear days (Ks 〉 0.8), these percentages ranged between 4.0% and 4.5% in Lhasa and between 5.1% and 5.5% in Haibei. In the case of cloudy days (Ks 〈 0.4), these percentages ranged from 4.4% to 6.8% in Lhasa and from 5.1% to 5.5% in Haibei. The maximum values of UV radiation for each relative optical mass diminished exponentially with mr. Thus, for Lhasa and Haibei, UV=46.25mr-129, and UV=51.76mr-142, respectively. The results of this study can be used to obtain more UV radiation data for the study of UV climate characteristics, the effects of UV on ecological processes and the feedback of the thinning of the stratospheric ozone, from more routine measurements Rs data.  相似文献   

14.
Summary ?The relationship between global photosynthetically active radiation (PAR) and global solar radiation is studied with a 2-year data archive of hourly values HPAR and HSW of these irradiances obtained at Athalassa, Cyprus. These data are used to determine the temporal variability of HPAR and its dependence on sky conditions. The seasonal variation of the ratio HPAR/HSW obtained from daily data ranges from 0.456 (during summer) to 0.451 (during winter) with an annual mean value of 0.454. The ratio increases from 0.454 to 0.467 (daily values) or from 0.460 to 0.501 (hourly values), as sky conditions change from clear to overcast. Finally, the effect of aerosol content on the HPAR/HSW ratio is found to incur substantial changes in the PAR fraction. Received June 27, 2001; revised April 17, 2002; accepted May 18, 2002  相似文献   

15.
In this study,the clear sky hourly global and net solar irradiances at the surface determined using SUNFLUX,a simple parameterization scheme,for three stations(Gaize,Naqu,and Lhasa) on the Tibetan Plateau were evaluated against observation data.Our modeled results agree well with observations.The correlation coefficients between modeled and observed values were > 0.99 for all three stations.The relative error of modeled results,in average was < 7%,and the root-mean-square variance was < 27 W m 2.The solar irradiances in the radiation model were slightly overestimated compared with observation data;there were at least two likely causes.First,the radiative effects of aerosols were not included in the radiation model.Second,solar irradiances determined by thermopile pyranometers include a thermal offset error that causes solar radiation to be slightly underestimated.The solar radiation absorbed by the ozone and water vapor was estimated.The results show that monthly mean solar radiation absorbed by the ozone is < 2% of the global solar radiation(< 14 W m 2).Solar radiation absorbed by water vapor is stronger in summer than in winter.The maximum amount of monthly mean solar radiation absorbed by water vapor can be up to 13% of the global solar radiation(95 W m 2).This indicates that water vapor measurements with high precision are very important for precise determination of solar radiation.  相似文献   

16.
Summary Thin plate smoothing splines incorporating topographic dependence were used to interpolate daily global solar radiation in the Bavarian forest ecosystem monitoring network, with the degree of data smoothing determined by minimizing the generalized cross validation. A simple cross validation method was used to discuss the spatial distribution of mean relative errors at 18 forest climate stations. The results show that, from this network 14%–30% mean relative errors can be expected for most of these forest climate stations in summer, and 20%–30% mean relative errors can be found at a few of forest climate stations in winter. Time-averaging can reduce these interpolation errors. In this network a mean relative error of 10% can be expected for weekly and biweekly mean solar radiation at most of forest climate stations in summer. Large errors are related to low radiation amount under heavy cloud cover. Mean relative errors increase as daily global solar radiation decreases. Received April 20, 1999 Revised January 20, 2000  相似文献   

17.
复杂地形对计算地表太阳短波辐射的影响   总被引:18,自引:2,他引:16  
首先利用数字高程数据(DEM)、大气辐射传输模式6S以及野外观测资料计算了复杂地形(青藏高原)上地表入射太阳辐射,然后计算不考虑地形产生的地表辐射的计算误差,对误差进行归一化后得到相对辐射误差.结果显示,相对辐射误差的标准差(即相对地表辐射计算误差绝对值的统计平均值) Se随太阳天顶角的增加呈指数增长,随高度标准差的增加几乎呈线性增长,随数字高程数据的分辨率(或卫星资料的分辨率)降低而降低.利用分步拟合方法拟合了Se随太阳天顶角、高度标准差和数字高程分辨率的变化.利用拟合方程可以计算任意地形条件下,不同分辨率的卫星(或数字高程)资料在不同太阳天顶角情况下,不考虑地形复杂性产生的平均地表入射太阳辐射的计算误差,结果表明,使用中分辨率的卫星(如MODIS)资料计算地表太阳净辐射时,需要考虑地形复杂性.  相似文献   

18.
Based on the analysis of one year of observation data of solar radiation at the ground in Beijing in 1990, a simple empirical formula for calculating UV radiation in overcast sky is established. The formula is Qlw/Quvo = A1S Ao, where Quv and Quvo are monthly mean daily sums of UV exposure in overcast sky and clear sky, respectively. S is the daily sunshine hours. The calculated results agree well with the observed. The maximum and minimum relative biases are 9.9% and 0.1%, respectively, and the yearly relative bias is 2.9%. The ratio of ultraviolet radiation of overcast sky to clear sky in 1990 is between 44.6% and 61.8%, and the yearly average is 53.9%. Thus, almost half of the UV energy is lost in the atmosphere in overcast sky in 1990.  相似文献   

19.
山西省太阳能资源时空分布特征及利用潜力评估   总被引:2,自引:0,他引:2  
按照中国气象局发布的太阳能资源评估方法,利用山西省近30 a 3个辐射观测站的太阳总辐射资料和105个站的日照资料,采用气候学方法计算了山西省的太阳总辐射,在分析山西省太阳总辐射的空间分布和时间演变特征的基础上,计算了山西省太阳能资源的各种参数,对区域太阳能资源潜力进行了客观评估。结果表明山西省太阳能资源储备丰富、稳定、可开发利用日数较多,特别是山西北部地区,尤其适合进行太阳能资源开发利用。  相似文献   

20.
中国地表太阳辐射再分析数据与观测的比较   总被引:3,自引:1,他引:2       下载免费PDF全文
利用我国地表太阳辐射台站资料和海上观测资料与同期的NCEP/NCAR, NCEP/CFSR再分析资料进行比较,检验再分析资料是否能够反映中国地区的太阳辐射特征。结果表明:1979年之前NCEP/NCAR太阳辐射资料的可信度较低,存在虚假的明显上升趋势,1979年之后两套再分析资料的可信度均较高,在我国东部和低纬度地区的可信度好于西部和高纬度地区;由逐6 h再分析数据直接计算得到的逐日太阳辐射比实际观测偏低,剔除太阳辐射为零的情况计算逐日资料更合理。在大陆地区,NCEP/NCAR,NCEP/CFSR再分析资料与台站太阳辐射资料的1979—2009年共31年平均误差分别为10.37 W·m-2和-42.68 W·m-2,误差的标准差分别为12.31 W·m-2和4.19 W·m-2;在海洋区域,NCEP/NCAR,NCEP/CFSR再分析资料与海上观测太阳辐射资料的平均误差分别为-161.19 W·m-2和-179.66 W·m-2,误差的标准差分别为37.07 W·m-2和35.36 W·m-2。与大陆台站资料相比,海上观测与再分析资料的误差偏大,这可能与海上观测资料较少,限制了NCEP模式的评估和改进有关。  相似文献   

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