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1.
拉萨紫外辐射特征分析及估算公式的建立 总被引：2，自引：1，他引：1
本文利用2005~2010年的辐射观测资料对拉萨地区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,结果表明,紫外辐射与太阳总辐射的变化规律基本一致,日变化表现为正午大、早晚小;季变化特征是夏季6月最大,冬季1月最小.紫外辐射日累积值6年平均为0.87 MJ·m-2·d-1;紫外辐射有逐年递减的趋势.紫外辐射与总辐射比值也存在着明显日变化,表现为正午大、早晚小的规律;其季节变化也是夏季最大,冬季最小.紫外辐射与总辐射比值6年平均为0.0418;紫外辐射与总辐射比值也呈现逐年递减的趋势.利用2010年大气质量数和晴空指数,建立了适合于拉萨紫外辐射估量的公式,估算值的瞬时值与观测值的平均相对误差最大为8.66%,紫外辐射日累积重构值与观测值平均相对误差仅为5.5%. 相似文献
2.
山东禹城紫外辐射变化特征及其估测方程的建立 总被引：1，自引：0，他引：1
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。 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
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.
利用2005~2011年的太阳辐射观测资料分析三江平原地区光合有效辐射(Qp)的时间变化特征及其与总辐射(Rs)比值(Qp/Rs)的变化规律,结果表明,Qp与Rs具有相同的季节变化特征;Qp日累计值的变化范围为60.47~0.11 mol m-2 d-1,年均值为23.76 mol m-2 d-1。Qp/Rs的变化范围为1.52~2.07 mol MJ-1,年均值为1.91 mol MJ-1。Qp/Rs和Qp季节变化一致,两者都是夏季最大,春秋次之,冬季最小。通过利用2011年的Qp观测数据、大气质量数与晴空指数的相互关系,建立了适合于估量三江地区Qp的经验方程,估算值与观测值的相对误差在5.7%以内。 相似文献
5.
拉萨光合有效辐射的变化趋势及其估算方程的建立 总被引：3，自引：0，他引：3
利用2005年1月-2010年12月中国生态研究网络拉萨农田站的观测数据,分析了拉萨地区光合有效辐射Qp的变化特征.结果表明,拉萨地区的Qp与太阳总辐射Rs具有相同的月变化和日变化特征,Rs与Qp的平均日累计值分别为20.2 MJ·m-2和37.2 mol·m-2,Qp呈逐年递减趋势.Rs与Qp的月变化表现为6月最大、1月最小,其最大、最小值分别为25.4 MJ·m-2、14.0 M J·m-2和48.7 mol·m-2、25.2 mol·m-2.日变化表现为正午大、早晚小.光合有效辐射系数(Qp/Rs)的变化范围在1.3～3.2 mol·MJ-1之间,年平均值为1.89 mol·MJ-1,呈逐年递减趋势,2010年比2005年降低了6.7％.Qp/Rs的日变化表现为早晚大、正午小,季节变化表现为夏季最大、春秋季次之、冬季最小,而且夏、冬两季的季节变化较为明显,冬季比夏季低10.6％.通过分析Qp与晴空指数和太阳天顶角之间的关系建立了拉萨地区Qp的估算方程,相对误差在4.49％左右. 相似文献
6.
香河地区光合有效辐射观测分析研究 总被引：3，自引：0，他引：3
利用中国科学院大气物理研究所香河大气综合观测实验站(39°47′N,116°57′E)2004年10月至2005年12月共15个月的太阳辐射观测资料,分析了该地区光合有效辐射与太阳总辐射比值的(PAR/Rs)日变化和季节变化特征,得出月平均PAR/Rs值变化范围在1.808~2.048μE.J-1之间,最大值出现在夏季,最小值出现在冬季,年平均值为1.948μE.J-1。提出了一个利用太阳总辐射观测值计算光合有效辐射瞬时值的参数化算式,用该算式计算得到的PAR与实际观测值的均方根误差为19.28μE.m-2.s-1,有96%的计算值与观测值偏差在±10%以内。比较了香河地区与太湖地区、额济纳地区光合有效辐射瞬时最大值、小时累积最大值及日累积最大值的差异。 相似文献
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8.
HEIFE绿洲区太阳总辐射和地表反射率的分光谱特征 总被引：3，自引：0，他引：3
太阳辐射的分光测量在许多研究和应用领域中都具有十分重要的意义．本文利用HEIFE临泽子站进行的太阳总辐射和反射辐射的分光观测资料，研究了黑河绿洲区太阳总辐射和地表反射率的光谱特征．研究结果表明：在太阳总辐射的光谱能量分布中，紫外和可见光部分的比倒偏小，近红外部分则偏太．在其从冬到夏的季节变化中紫外和可见光部分是由小到大，近红外部分剐是由大到小。在其日变化中0．5μm以下波段是中午大早晚小；0．7μm以上波段是中午小，早晚大；0．5-0．7μm波段的日变化不明显。紫外波段的相对日变化幅度最大．地表反射率的光谱特性有明显的季节变化，变化特征与地表植被状况有关．各波段地表反射率的日变化型有一定的季节差异，其中波长小于0．7μm部分较为明显，并与地表植被状况有关．在裸露地表各波段反射率与太阳高度角的关系中，近红外波段随太阳高度角增加而增大，紫外和可见光波段则随太阳高度角增大而减小．全波段反射率随太阳高度角增大而增大主要是近红外波段的贡献．这是裸露地表光谱反射率的重要特征之一。 相似文献
9.
NO2的光解速率j(NO2)是对流层化学研究中的一个重要的参数，它是对流层臭氧（O3）和OH自由基的形成关键影响因子之一。本文利用香河站2017年11月至2018年1月的观测资料对NO2的光解速率j(NO2)、太阳辐射的变化特征，及光解速率与分波段辐射相关性进行分析，在此基础上建立了一套适合于构建香河地区j(NO2)的参数化方案。结果表明，香河地区的j(NO2)与太阳辐射的变化趋势基本一致，日变化均呈正午高、早晚低的单峰型。香河地区冬季j(NO2)的变化范围是0.00046～0.0044 s-1，平均值为0.0029 s-1。j(NO2)与晴空指数（KS）和定义的紫外辐射晴空指数（KUV）存在很好的相关性，因此，利用j(NO2)与大气质量数和晴空指数的相互依赖关系，基于KUV构建了适合于香河地区j(NO2) 的估算方程。由于总辐射是气象站的常规观测要素，晴空指数KS更容易获取，继而建立了通过KS参数化计算j(NO2)的估算方程。利用KUV和KS建立的j(NO2)估算方程的瞬时估算值与观测值的平均相对误差分别为6.5%和13.9%，均方根误差分别为0.00029和0.00051。 相似文献
10.
根据1996～1998年由NILUV紫外辐射仪在西藏拉萨地区观测的紫外辐射资料,分析了青藏高原拉萨地区生物有效辐射的分布特征.结果表明,1997年日正午最大生物有效紫外辐射剂量率(UV dose rate)达到500mW m-2,最小值为9.7 mW m-2;晴天时生物有效辐射剂量率的日变化呈规则曲线,且早晚小,中午大;一年中紫外辐射变化的总趋势是由太阳天顶角决定的,紫外辐射的日变化和年变化是其最主要、最基本的变化;西藏拉萨地区的月平均红斑辐射剂量明显高于全球其他同纬度地区. 相似文献
11.
Measurements of broadband global solar and ultraviolet radiation (UV-KZ) by a Kipp & Zonen radiometer from 2005 to 2011 at three sites in the background region over Northeast China were used to investigate the characteristics of the temporal variability of UV-KZ radiation in Northeast China. The highest annual mean daily values of UV-KZ (0.53 MJ m?2 d?1) were observed at Sanjiang and Changbai Mountain. The lowest value (0.49 MJ m?2 d?1) was measured at Hailun due to the high aerosol burden and the long path of solar radiation. The diurnal variation in UV-KZ radiation on four clear days near the equinoxes and solstices exhibited bell-shaped curves, with a maximum at approximately noon. There was little difference in UV-KZ radiation between representative spring and autumn days except that the amount of UV-KZ radiation during the spring was higher than that during the autumn. The relationship between the maximum values of UV-KZ radiation and clearness index can be accurately demonstrated with three polynomial equations. An empirical estimation model suited for all weather conditions was developed using measurements collected at Hailun. The slope of the linear regression between the measured and modeled UV-KZ radiation was approximately 1, the intercept of the linear regression equation was near zero, and the relative error of the equation was less than 8.5 %. These validation results suggest that this model can accurately estimate the UV-KZ radiation based on more conventional measured radiation data. The empirical estimation model can also serve as a valuable method for the study of ecological processes in other regions. 相似文献
12.
Measurements of the broadband global solar radiation (R S) and total ultraviolet radiation (the sum of UV-A and UV-B) were conducted from 2005 to 2010 at 9 sites in arid and semi-arid regions of China. These data were used to determine the temporal variability of UV and UV/R S and their dependence on the water vapor content and clearness index. The dependence of UV/R S on aerosol optical depth (AOD) and water vapor content was also investigated. In addition, a simple and efficient empirically model suited for all-weather conditions was developed to estimate UV from R s. The annual average daily UV level in arid and semi-arid areas is 0.61 and 0.59 MJ m?2 d?1, respectively. The highest value (0.66?±?0.25 MJ m?2 d?1) was recorded at an arid area at Linze. The lowest value (0.53?±?0.22 MJ m?2 d?1) was recorded at a semi-arid area at Ansai. The highest daily value of UV radiation was measured in May, whereas the lowest value was measured in December. The monthly variation of the UV/R s ratio ranged from 0.41 in Aksu to 0.35 in Qira. The monthly mean value of UV/R s gradually increased from November and then decreased in August. A small decreasing trend of UV/R s was observed in the arid and semi-arid regions due to recently increasing amounts of fine aerosol. A simple and efficient empirically model suit for all-weather condition was developed to estimate UV from R s. The slope a and intercept b of the regression line between the estimated and measured values were close to 1 and zero, respectively. The relative error between the estimated and measured values was less than 11.5%. Application of the model to data collected from different locations in this region also resulted in reasonable estimates of UV. 相似文献
13.
Lili Jin Qing He Zhenjie Li Rui Liu Ali Mamtimin Qilong Miao 《Meteorology and Atmospheric Physics》2014,126(1-2):91-103
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. 相似文献
14.
In situ measured data of broadband solar radiation （Rs） and ultraviolet （Uv） radiation were used to investigate the spa- tiotemporal variation properties of Uv radiation and the ratio of Uv radiation to Rs over the North China Plain （NCP）. Based on the analysis, an empirical model for estimating Uv radiation under all weather conditions in this region was developed. The results showed that the annual Uv radiation over the NCP ranges from 0.38-0.52 MJ m^-2 d^-1. The highest value during the study period was recorded at the Changwu site, which is located near the margin of the Loess Plateau, while the lowest value appeared at the station in Beijing. The seasonal variation pattern of the ratio of Uv radiation to Rs is similar to that of Uv radiation; namely, the highest value appears in August and then decreases gradually until the lowest value appears in November. A small increasing trend in the Uv radiation levels and the ratio of Uv radiation to Rs was observed over the NCP. The evaluation results showed that the empirical estimation model can be widely used to estimate Uv radiation under all atmospheric conditions. The relative error between the modeled and measured daily values were within ± 15%. 相似文献
15.
杜军剑 《沙漠与绿洲气象(新疆气象)》2013,7(4):45-50
基于焉耆国家基准气候站1993-2012年逐月太阳总辐射和日照观测资料以及和静、巴音布鲁克1961-2012年月日照百分率资料,建立回归分析方程,推算和静县山区及平原地区逐月的太阳总辐射,对比分析了和静县山区及平原地区太阳总辐射变化特征,从太阳能资源丰富度、资源稳定性及可利用价值等方面对和静县太阳能资源状况进行评估。结果表明：1961-2012年和静县平原及山区太阳总辐射均呈减少的趋势,平原地区7月太阳总辐射最多,山区5月最多,最少值均出现在1月;平原地区属太阳能资源很丰富区,山区为丰富区;平原地区及山区太阳能资源均较稳定;平原地区年平均可利用太阳辐射的天数为286 d,山区为267 d;平原和山区一天中上午和中午是最有利的利用时段。 相似文献
16.
An updated version of the Regional Acid Deposition Model(RADM)driven by meteorologicalfields derived from Chinese Regional Climate Model(CRegCM)is used to simulate seasonal variationof tropospheric ozone over the eastern China.The results show that:(1)Peak O_3 concentration moves from south China to north China responding to the changing ofsolar perpendicular incidence point from south to north.When solar perpendicular incidence pointmoves from north to south,so does the peak O_3 concentration.(2)In the eastern China.the highest O_3 month-average concentration appears in July.thelowest in January and the medium in April and October.The pattern mainly depends on the solarradiation,the concentration of O_3 precursors NO_x and NMHC and the ratio of NMHC/NO_x.(3)Daily variations of O_3 over the eastern China are clear.Namely,O_3 concentrations rise withthe sun rising and the maximums appear at noon.then O_3 concentrations decrease.The highest dailyvariation range of O_3 appears in summer(40×10~(-9) in volume fraction)and the lowest in winter(20×10~(-9) in volume fraction).(4)Daily variations of O_3 over the western China are not clear.The daily variation range of O_3 isless than 10×10~(-9) in volume fraction. 相似文献