藏北高原地表反照率的初步研究

基于中日合作项目“全球协调加强观测计划之亚澳季风青藏高原试验”(CAMP/Tibet)在藏北高原D105站、Amdo站、MS3478站以及BJ站的观测数据资料,分析了该地区地表反照率的时空分布特征。结果表明:藏北高原地区的地表反照率具有明显的日变化和月/季节变化特征。冬、春季的日变化曲线呈“U”形,且曲线形状的变化不如夏、秋季大。6~9月的月平均反照率在全年中最低,5月份月平均反照率波动较大。从季节平均值来说,冬季>春季>秋季>夏季。该地区的平均地表反照率为0.2457;反照率的空间分布很不均匀,其值的大小、曲线的形状在不同站点都很不一样,这与站点的地理位置有关,但天气状况和下垫面属性也起了很大的作用。     

藏北高原地面加热场的变化及其对气候的影响

利用 1994— 1996年在藏北高原五道梁所观测得到的地面能量收支资料 ,结合同期的大气环流进行了分析研究。结果表明 :高原北部地面加热场强度的变化与高原西部相似 ,而与高原主体东半部的变化相反 ;冬季前期 11月的地面积雪过程对决定整个冬季地面加热场的性质具有重要的意义 ;高原冬季地面热状况的异常 ,引起夏季加热场的异常 ,这可能是造成大气环流异常的原因之一 ,从而影响我国的气候环境 ,因此对高原地面加热场的监测可以为短期气候预测提供依据。     

藏北高原地面加热场的季节变化

利用五道梁１９９３年９月～１９９５年８月的辐射收支资料，分析了该地区地面加热场的季节变化特征，结果表明：春，秋季地面加热场强度有明显的急增加减过程，正是加热场的这种突变引起了季节的明显转换，冬季地面积雪多的年从那面加热场强度较弱，第二年夏季加热场强度则较强；地面加热场强度的季节变化明显，夏季强，冬季弱；冬季地面积雪时间较长时，由于地表反射率增大，地中释放的土壤热通量较无雪时减少，可能造成该地区地面     

东帕米尔高原地表辐射收支及地表反照率特征

利用东帕米尔高原塔什库尔干国家基本气候站2020年6月至2021年6月观测的辐射数据,分析了东帕米尔高原不同时间尺度和不同天气条件下各辐射通量及地表反照率变化特征。结果表明：（1）各辐射通量在逐日均值变化上呈“V”型曲线;向下短波辐射、向上短波辐射、向下长波辐射、向上长波辐射和净辐射年曝辐量分别为5001.6, 1370.3, 6090.7, 8550.8和1189.0 MJ·m-2;在季节尺度上,各辐射通量总体表现为夏季>春季>秋季>冬季,而向上短波辐射在冬季最高。（2）不同天气下,辐射通量也不同,晴天时,各辐射通量变化均为较平滑的单峰型,少云、多云时均为不规则单峰型,降水时,除冬季外均为多峰型,辐射通量均值变化表现为晴天>少云>多云>降水。（3）地表反照率在观测期间平均值为0.29,最大值出现在1月,最小值出现在7月,分别为0.58和0.24;在季节上表现为冬季最大,夏季最小;春、夏、秋季地表反照率呈“U”型,冬季为倒“U”型;降雨时地表反照率下降,降雪时则地表反照率上升,说明不同降水类型对地表反照率影响不同。     

玛曲高寒草甸地表辐射与能量收支的季节变化

利用中国科学院黄河源区气候与环境综合观测研究站2010年观测资料,分析了玛曲高寒草甸地表辐射与能量收支的季节特征。结果表明:玛曲高寒草甸入射太阳辐射与净辐射年累积量分别为6482.2和2577.2MJ.m-2.a-1;年平均地表反照率为0.25,生长期平均地表反照率为0.22;全年入射太阳辐射的38%转换为地表长波辐射,明显高于低海拔地区的草地;净辐射占入射太阳辐射的38%,低于全球以及低海拔地区的草地;在冻结期,感热通量占净辐射的93%,在生长期,潜热通量占净辐射的62%。     

巴丹吉林沙漠不同下垫面辐射特征和地表能量收支分析

利用2009年夏季在内蒙古自治区阿拉善右旗境内巴丹吉林沙漠开展的"巴丹吉林沙漠陆-气相互作用观测试验"所取得的资料,对比分析了典型晴天条件下,巴丹吉林沙漠两种不同下垫面的辐射平衡特征和地表能量收支的日变化规律。结果表明,不同下垫面地表反射率具有明显的差异,沙漠反射率为0.33,湖区沙生芦苇反射率为0.23,沙漠反射率大于沙生芦苇反射率。巴丹吉林沙漠两种典型下垫面上,各辐射分量均具有相似的日变化特征,即白天大、夜间小。两种下垫面上的净辐射日变化与峰值基本相同,日积分值均约为8MJ.m-2。由于下垫面性质不同,地表能量的分配也不相同。沙漠主要以感热通量为主,地表热流量其次,潜热通量很小可以忽略不计;湖区以潜热通量为主,感热通量和地表热流量次之。     

藏北高原那曲地区不同下垫面地表粗糙度的变化特征研究

利用2008年、2010年和2012年藏北高原那曲地区MODIS卫星数据和站点大气湍流观测数据,分别应用Massman反演模型和一种确定地表粗糙度的独立方法,计算并分析地表粗糙度的时空变化特征并对反演模型进行验证,分析Z0m存在着明显的季节性变化特征。2—8月伴随冰雪消融与植被生长,Z0m逐渐增大,站点Z0m最大可达4～5 cm。9月至次年2月由于高原季风的衰退期等原因,Z0m逐渐减小,站点Z0m减小至1～2 cm。异常年份的降雪是Z0m明显低于常年的主要原因。依据Z0m的由小到大可以将下垫面分为冰雪类、稀疏草地类、茂盛草地类、城镇类4类,其中茂盛草地类和稀疏草地类分别占区域62. 49%和33. 74%,为主要类别,其Z0m年变化分别在2～6 cm和1～4 cm之间。两种计算方法得出的结论相关性较好,由于平均滑动作用,反演资料较实测计算结果偏小。整体而言,利用卫星数据反演算法计算的Z0m是可行的,并可应用于改进陆面模式参数,提高模式模拟的准确性,能更好的揭示区域的热通量交换。     

藏北高原地表能量和边界层结构的数值模拟

利用耦合了NCAR LSM陆面过程的中尺度模式MM5V3.7和2002年8月CAMP/Tibet加强期的观测资料,对藏北高原地区地气交换过程进行了48 h模拟研究。模式较好地模拟了该地区的山谷风环流;并将模拟的地表通量在中尺度区域上与NCEP/NCAR全球大气再分析格点资料(NNRP)获得的结果进行了比较,同时也与单站的实测值进行了比较,结果显示:模拟的地表通量与NNRP得到的结果比较吻合,同时可以得到雨季时藏北、藏东地区潜热通量大于感热通量,而高原西部感热通量大于潜热通量,这与观测试验分析结果一致;与单站试验结果比较,模拟的感热通量与实测值一致,潜热通量的模拟值和实测值有一定差别。模拟的边界层位温廓线与实测值比较,模式模拟的对流混合层和夜间残留层都与实测结果吻合,但模拟的混合层高度较实测值高。由此来看,中尺度模式MM5V3.7能够较好地模拟藏北高原的地表能量和边界层结构特征,但还需要进一步完善陆面过程和物理过程参数化方案。     

青藏高原不同地区辐射特征对比分析

利用全球协调加强观测计划(CEOP)之亚澳季风青藏高原试验(CAMP/Tibet)在藏北高原的BJ站、NPAM站及中国科学院珠穆朗玛峰大气与环境综合观测研究站、纳木错多圈层相互作用综合观测研究站和藏东南高山环境综合观测研究站2007年的辐射观测资料,分析了这些地区不同下垫面地表辐射各分量及地表反照率的日变化和月际变化特征。结果表明,向下短波辐射受太阳高度角的影响存在明显的日变化和月际变化;向上短波辐射的月际变化基本与总辐射一致,在个别月份由于高原积雪造成地表反照率较高,从而使晴天向上短波辐射全年较高;向下长波辐射存在基本的季节变化,最大值出现在天空总云量较多的夏季(6～8月),最小值出现在冬季(12月和1月);向上长波辐射基本上都是夏季为全年最大,冬季为全年最小。这与地表温度的年变化情况相一致。高原不同地区各季节晴天地表净辐射存在差异,NPAM站和藏东南站由于下垫面植被覆盖较好,净辐射值各季节均高于其它各站;NPAM站、纳木错站和珠峰站地表反照率日变化曲线呈U型,BJ站和藏东南站日变化相对复杂,藏东南站全年月平均地表反照率较小且变化不大,其他各站存在基本的年变化趋势。     

藏北地区近地层大气和土壤特征量分析

利用"全球协调加强观测期亚澳季风青藏高原试验研究(CAMP/Tibet)"4个台站2003年大气和土壤的观测资料,详细分析了藏北高原不同下垫面上的气温、相对湿度、土壤温度、土壤湿度等的季节变化及年变化特征。近地层大气各气象要素变化剧烈;4个站气温高低的差异显示了纬度和高度的明显影响;各站冻土冻融过程存在地域差别,尤其是春季冻结消融阶段的持续时间相差可达1个月;土壤质地的差别对土壤湿度影响也较大,黏土土壤含水量要高些,粉土和砂土要低些。     

地表反照率与高原夏季风爆发关系分析

利用2000～2016年MODIS地表反照率和ECMWF/ERA-Interim再分析资料,选取有代表性的高原季风指数DPMI,统计分析了青藏高原地表反照率与高原季风之间的联系,结果表明:1)11月高原地表反照率大小与次年高原夏季风爆发存在密切关系:11月高原地表反照率偏低(高),次年4月高原夏季风爆发偏早(晚),强度偏强(弱)。2)可能的影响机制为:当前期11月高原地表反照率偏低时,后期高原主体对大气的感热加热信号更强,从而引起4月高原上空近地面层上升运动明显加强,这有利于热量向高空传输,导致对流层加热作用加强,高原上空对流层温度偏高,使得高原季风环流系统加强,最终导致高原季风季节变化相应提前;反之亦然。     

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.     

Estimation of Hourly Solar Radiation at the Surface under Cloudless Conditions on the Tibetan Plateau Using a Simple Radiation Model

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.     

夏季青藏高原地面热源和高原低涡生成频数的日变化

通过1981—2010年NCEP/NCAR再分析资料,分析出夏季青藏高原地面热源具有强烈的日变化,白天高原是强热源,夜间高原地面转变为弱热汇,日较差可达420 W·m~(-2),呈由西向东递减分布。其中地面感热和潜热加热的日变化均十分明显,日较差分别可达300 W·m~(-2)和200 W·m~(-2);感热加热的日变幅由西北向东南递减,而潜热加热由南向北递减。同时,利用人工识别的高原低涡数据集初步分析了夏季高原低涡生成频数的日变化,发现夜间生成的高原低涡频数略高于白天,其中00 UTC的低涡源地主要在西藏那曲和林芝(工布江达),12 UTC低涡源地主要在西藏那曲和青海玉树。     

A Study on Parameterization of Surface Albedo over Grassland Surface in the Northern Tibetan Plateau

The relationship of surface albedo with the solar altitude angle and soil moisture is analyzed based on two-year (January 2002 to December 2003) observational data from the AWS (Automatic Weather Station) at MS3478 in the northern Tibetan Plateau during the experimental period of CEOP/CAMP-Tibet (Coordinated Enhanced Observing Period Asia-Australia Monsoon Project on the Tibetan Plateau). As a double-variable (solar altitude angle and soil moisture) function, surface albedo varies inconspicuously with any single factor. By using the method of approximately separating the double-variable function into two, one-factor functions (product and addition), the relationship of albedo with these two factors presents much better. The product and additional empirical formulae of albedo are then preliminarily fitted based on long-term experimental data. By comparison with observed values, it is found that the parameterization formulae fitted by using observational data are mostly reliable and their correlation coefficients are both over 0.6. The empirical formulae of albedo though, for the northern Tibetan Plateau, need to be tested by much more representative observational data with the help of numerical models and the retrieval of remote sensing data. It is practical until it is changed into effective parameterization formulae representing a grid scale in models.     

青藏高原地区地表及行星反射率

文章讨论了利用ISCCP卫星观测资料确定青藏高原地区地表反射率的方法,在无积雪地区和季节,地表反射率可以ISCCP可见光反射率为基础,在模式计算过程中,假定紫外反射率以及红外与可见光反射率的比值分别为常数。敏感性试验表明,由这两个假设所产生的误差并不显著。在有积雪地区或季节,地表平均反射率可直接由ISCCP可见光反射率表示。试验结果与地面实际观测作了比较,除沙漠区外,两者比较一致。文中还计算了高原晴天行星反射率。经与ERBE卫星观测比较,发现从5月至9月高原周围沙漠区气溶胶对辐射平衡有较显著的影响。而在其     

Surface Flux Parameterization in the Tibetan Plateau

This study investigates some basic aspects related to surface-flux parameterization in the Tibetan Plateau, based on the measurement at three sites. These sites are essentially flat and covered by very sparse and short grasses in the monsoon season. The main contributions include: (1) an optimization technique is proposed to estimate aerodynamic roughness length based on wind and temperature profiles. The approach is not sensitive to random measurement errors if the number of data samples is large enough. The optimized values reasonably vary with surface characteristics. (2) At the three sites, kB^-1 (the logarithm of the ratio of aerodynamic roughness length to thermal roughness length) experiences seasonal and diurnal variations in addition to a dependence on surface types. The mean values for the individual sites vary over a range of 2.7 to 6.4 with large standard deviations. (3) A formula for estimatingthe value of kB^-1 isproposed to account for the effect of seasonal variation of aerodynamic roughness length and diurnal variation of surface temperature. With the formula, the flux parameterization with surface temperature estimates sensible heat flux better than profile parameterization for all the sites.     

Air Temperature Estimation with MODIS Data over the Northern Tibetan Plateau

Time series of MODIS land surface temperature(T_s) and normalized difference vegetation index(NDVI) products,combined with digital elevation model(DEM) and meteorological data from 2001 to 2012,were used to map the spatial distribution of monthly mean air temperature over the Northern Tibetan Plateau(NTP). A time series analysis and a regression analysis of monthly mean land surface temperature(T_s) and air temperature(T_a) were conducted using ordinary linear regression(OLR) and geographical weighted regression(GWR). The analyses showed that GWR,which considers MODIS T_s,NDVI and elevation as independent variables,yielded much better results [R_(Adj)~2 0.79; root-mean-square error(RMSE) =0.51℃–1.12℃] associated with estimating T_a compared to those from OLR(R_(Adj)~2= 0.40-0.78; RMSE = 1.60℃–4.38℃).In addition,some characteristics of the spatial distribution of monthly T_a and the difference between the surface and air temperature(T_d) are as follows. According to the analysis of the 0℃ and 10℃ isothermals,T_a values over the NTP at elevations of 4000–5000 m were greater than 10℃ in the summer(from May to October),and T_a values at an elevation of3200 m dropped below 0℃ in the winter(from November to April). T_a exhibited an increasing trend from northwest to southeast. Except in the southeastern area of the NTP,T d values in other areas were all larger than 0℃ in the winter.