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1.
玛曲高寒草甸地表辐射与能量收支的季节变化 总被引：3，自引：0，他引：3
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%。 相似文献
2.
利用TUV模式计算分析了银川光化辐射通量变化特征,探讨了云、气溶胶、臭氧柱浓度、NO_(2)柱浓度等因子对银川光化辐射通量的影响。结果表明:2019年7—9月银川月平均光化辐射通量分别为6.5E+16光子数·cm^(-2)·s^(-1)、5.6E+16光子数·cm^(-2)·s^(-1)和4.7E+16光子数·cm^(-2)·s^(-1),日最大值出现在13:00;波长小于325 nm时,光化辐射通量随波长增加缓慢上升,波长在325—480 nm之间时,光化辐射通量迅速升高,波长大于480 nm时,光化辐射通量随波长增加变化较小,此特征在中午前后较早晚表现更明显;云光学厚度和气溶胶光学厚度对光化辐射通量的衰减作用具有明显的“U”型日变化特征,比较而言,气溶胶光学厚度对光化辐射通量衰减作用的“U”型波形更为宽广;光化辐射通量衰减率对较低的云光学厚度的变化更敏感;光化辐射通量随气溶胶光学厚度增加而减小的变率要比随云光学厚度增加而减小的变率小;光化辐射通量对单次散射反照比大于0.6的强散射性气溶胶的变化更敏感,且气溶胶光学厚度越大,此特性整体表现越明显;波长指数对光化辐射通量的影响相对较小。 相似文献
3.
辐射和积云对流过程对大气辐射通量的影响 总被引：4，自引：1，他引：3
基于中国科学院大气物理研究所大气科学和地球流体力学数值模拟国家重点实验室发展的全球大气环流谱模式(SAMIL-R42L26),研究了澳大利亚气象局研究中心(BMRC)新辐射方案和新Zhang-McFaflane积云对流方案对大气辐射通量模拟的影响.新辐射方案相比原辐射方案在辐射计算光谱分辨率、气体吸收和计算效率等方面作了很多改进,其对大气辐射通量的模拟能力相应提高.在晴空条件下,大气顶出射长波、大气吸收短波和地表入射短波等与观测的偏差较原辐射方案明显减小,尤其是在对流活跃区域.在云天条件下大气辐射通量与观测的偏差也较原辐射方案减小,但其偏差依然较大,这与模式中积云对流参数化方案模拟能力不足引起的辐射通量偏差有关.为此,换用了新Zhang-McFarlane积云对流方案,其结果表明,对流活跃区水汽含量显著增加,原对流方案中偏强的"双赤道辐合带"现象明显减弱,赤道辐合带地区的大气辐射通量偏差有明显减小,在海洋地区晴空大气顶出射长波和地表入射短波的量值及空间分布均接近观测结果,同时大气顶全球平均能量收支的年变化和观测结果趋于一致,其中模拟的伞球年平均大气顶能量收支和观测的偏差不到0.6 W/m2.试验结果同时表明,在未来研究中引入气溶胶分布、调整相关的云物理和陆面过程等物理参数化方案是进一步提高SAMIL-R42L26辐射通最模拟性能的关键. 相似文献
4.
对青藏高原地区地表能量的研究是一个十分重要的问题.利用中国科学院珠穆朗玛峰大气与环境综合观测研究站2006年5月至2007年4月一年的观测资料,分析了青藏高原珠峰地区的地表能量,即净辐射通量、感热通量、潜热通量和土壤热通量,得到了一些有关珠峰地区地表能量的结果,即太阳总辐射、大气长波辐射、地面长波辐射和净辐射呈现出明显的年变化特征,净辐射、感热通量、潜热通量和土壤热通量得到的日变化是很明显的.并且讨论了计算地表能量通量的方法及其优缺点. 相似文献
5.
陆面模拟中植被辐射传输参数化方案研究 总被引：2，自引：0，他引：2
在冠层二流辐射传输模式基础上新发展了一个描述太阳短波辐射在植被中传输的冠层四流辐射传输模式.冠层四流辐射传输模式是在大气辐射传输理论的基础上得到一组描述短波辐射在植被中传输过程的冠层辐射传输基本方程,引进大气中求解辐射传输方程的四流近似解法,并求得冠层四流辐射传输方程的解析解.方程中各项参量能够反映叶子或冠层特殊的几何和光学特征.冠层向上、向下辐射通量取决于冠层散射相函数、叶子在入射光方向投影面积、单个叶子反射率和透射率、叶面积指数以及直射光入射太阳高度角等.四流模式计算叶子水平倾角时对太阳短波辐射的反照率,与二流模式结果比较可以验证模式的理论推导和建模都是正确的:计算结果的比较,表明四流模式在水平叶角分布时计算的冠层反照率与二流模式结果一致,同时直射光从任何太阳高度角入射的冠层反照率结果也一致,从而证明发展的冠层四流辐射传输模式是成功的.模拟试验中将两种模型同时耦合到同一个陆面过程模式中进行比较试验,结果表明,冠层四流辐射传输模式能够得到更精确的植被反照率,从而使得陆面模式计算的地表吸收的净太阳辐射通量更接近于观测值. 相似文献
6.
HUBEX试验区近地面层的湍流输送 总被引：8，自引：1，他引：7
1998年淮河流域能量和水循环试验(HUBEX)期间曾进行了1个月的近地面层湍流观测.分析不稳定条件下湍流的统计特性和谱特征,并与Monin-Obukhov相似理论进行了比较.结果表明,不稳定的时候各湍流量的统计特征与相似理论的预期相符.虽然不稳定条件下温度和湿度涨落的相关系数很高,谱的式样也相近,但湿度谱的峰值频率高于温度谱.协谱曲线的形状显示感热通量的谱峰较宽,表现出w和T在较宽范围的强相关性,而水汽通量谱在高频段下降很快,说明水汽的输送更多地出现在低频部分.从谱相关系数可见,在近中性的时候,各尺度湍流涡的热量输送效率普遍较低,随着不稳定性增强而显著提高.分析还发现,不论不稳定性的程度如何,小尺度湍流的水汽输送效率都较低.水汽通量谱的相关系数随稳定度的变化不如热通量的谱相关系数大,表明近中性时除小尺度湍流外其他湍流涡的水汽输送效率高于热量输送. 相似文献
7.
以云和地球辐射能量系统(CERES)数据集为准,量化了中国地球系统模式对地表入射短波辐射和大气逆辐射时空变化的模拟性能,明确了多模式间模拟结果存在不确定性的区域。结果表明：中国模式均能模拟出北半球地表入射短波辐射和大气逆辐射“夏高冬低”的季节变化特征。陆地上,中国模式对两个辐射分量月均值的模拟结果与CERES相当,在海洋上低于CERES结果。中国模式能模拟出地表入射短波辐射下降、大气逆辐射上升的年际变化趋势。对于2001—2014年均值,中国模式模拟的地表入射短波辐射在海洋和陆地上较CERES分别偏低3.3和3.0 W·m-2,模拟的大气逆辐射在海洋上与CERES结果相当,在陆地上较CERES低1.3 W·m-2。除南北纬30°附近之外,中国模式在其他纬度均低估地表入射短波辐射,以热带和北极最为明显。模式对大气逆辐射的模拟偏差呈纬向波动特征,模拟误差大值出现在高大山脉处。中国模式模拟地表入射短波辐射不确定性极大的区域分布在热带雨林和南极洲沿海,模拟大气逆辐射不确定性极大的区域分布在格林兰岛、青藏高原、安第斯山脉和南极洲沿海。 相似文献
8.
《干旱气象》2020,(1)
利用塔克拉玛干沙漠大气环境综合观测试验站——塔中站2014年30 min步长实测数据,系统分析塔克拉玛干沙漠腹地地表辐射和能量平衡特征及小气候特征。结果表明:塔中地区辐射平衡和能量平衡各分量均表现为春、夏季较大,秋、冬季较小,并具有明显的日变化特征,峰值出现在12:00(地方时,下同)左右。该地区地表能量通量(净辐射通量、感热通量、潜热通量和土壤热通量)中,净辐射、感热通量和土壤热通量均在08:00开始上升,至14:00左右达到峰值,而潜热通量变化很小。感热通量为能量的主要消耗形式,春、夏、秋、冬四季分别占净辐射的百分比为44. 6%、68. 1%、55. 2%和55. 3%,其次为土壤热通量,仅有很少能量用于水的相变。云和沙尘对能量通量各分量有明显削弱作用。近地层空气温度白天随高度的增加降低,夜晚则随高度的增加升高,空气相对湿度也呈明显变化规律。近地层水平风速随高度增加明显增大,风向以东北风为主。 相似文献
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利用"中国干旱气象科学研究计划——我国北方干旱致灾过程及机理"的观测数据,分析塔中站、奈曼站、平凉站和锦州站2015年8—10月及定西站2016年8—10月地表能量通量变化特征。分析发现,不同下垫面辐射均表现出明显的日变化,相对于向下短波辐射和向下长波辐射,不同下垫面反射辐射和向上长波辐射差异更加明显。塔中站反射辐射和向上长波辐射最大,锦州站和平凉站相对较小。净辐射具有明显的日变化特征,和总辐射相位一致,农田净辐射日峰值相对较大。地表反照率3个月平均从大到小依次为塔中站(0. 27)、定西站(0. 19)、锦州站(0. 16)、奈曼站(0. 15)和平凉站(0. 14)。各站点感热通量和潜热通量均为单峰型,其中,奈曼站感热通量峰值最大(276 W·m~(-2)),平凉站潜热通量峰值最大。定西站和锦州站净辐射分配以感热通量为主,平凉站则以潜热通量为主。 相似文献
11.
太阳散射辐射的分光测量及其能量分配 总被引：1，自引：0，他引：1
近十余年来，国内外不少学者先后研究了散射辐射与总辐射的关系［１－６］，建立了各种计算散射辐射的经验公式，但有关分光散射辐射分量的测量和研究为数甚少。为此，我们于１９８９－１９９０年在北京对３００－２８００ｎｍ光谱范围内的７个波段的散射分量进行测量，并研究了各分量与全谱段散射总量间的定量关系。 相似文献
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Francisco P. J. Valero Thomas P. Ackerman Warren J. Y. Gore 《Journal of Atmospheric Chemistry》1989,9(1-3):225-244
The interaction of the Aretic winter aerosol (Arctic haze) with solar radiation produces changes in the radiation field that result in the enhancement of scattering and absorption processes which alter the energy balance and solar energy distribution in the Arctic atmosphere-surface system. During the second Arctic Gas and Aerosols Sampling Project (AGASP II) field experiment, we measured radiation parameters using the NOAA WP-3D research aircraft as a platform. State-of-the-art instrumentation was used to measure in situ the absorption of solar radiation by the Arctic atmosphere during severe haze events. Simultaneously with the absorption measurements, we determined optical depths, and total, direct, and scattered radiation fields. All optical measurements were made at spectral bands centered at 412, 500, 675, and 778 nm and with a bandpass of 10 nm. With this selection of spectral regions we concentrated on the measurement of the radiative effects of the aerosol excluding most of the contributions by the gaseous components of the atmosphere. An additional measurement performed during these experiments was the determination of total solar spectrum fluxes. The experimentally determined parameters were used to define an aerosol model that was employed to deduce the absorption by the aerosols over the full solar spectrum and to calculate atmospheric heating rate profiles. The analyses summarized above allowed us to deduce the magnitude of the change in some important parameters. For example, we found changes in instantaneous heating rate of up to about 0.6 K/day. Besides the increased absorption (30 to 40%) and scattering of radiation by the atmosphere, the haze reduces the surface absorption of solar energy by 6 to 10% and the effective planetary albedo over ice surfaces by 3 to 6%. The vertical distribution of the absorbing aerosol is inferred from the flux measurements. Values for the specific absorption of carbon are found to be around 6 m2/g for externally mixed aerosol and about 11.7 m2/g for internally mixed aerosol. A complete study of the radiative effects of the Arctic haze should include infrared measurements and calculations as well as physics of the ice, snow, and water surfaces. 相似文献
15.
Tamio Takamura 《Boundary-Layer Meteorology》1992,59(1-2):67-82
The spectral reflectance of the surface in an urbanized area was estimated through airborne measurements of the spectral upward flux of visible radiation in the range 475–750 nm. Atmospheric effects due to Rayleigh and Mie scattering were accounted for by using optical parameters to solve the radiative transfer equation. The values for these parameters were derived from measurements of the particle number concentration and size distribution.The results clearly show a difference in reflectance between urban and suburban areas. The difference in spectral reflectance decreases from the suburban to the urban area.In a metropolitan area, the surface reflectance generally decreases with urban development, and the global upward flux of visible radiation has a similar tendency. This trend supports the idea of a decrease in reflectance due to the modification of the surface structure. 相似文献
16.
敦煌绿洲-戈壁过渡带地表辐射与能量特征分析 总被引：19，自引：11，他引：8
利用"西北干旱区陆-气相互作用野外观测试验"2002年在敦煌加强期的资料, 分析了敦煌绿洲-戈壁过渡带的地表辐射和能量特征.研究表明 白天, 绿洲-戈壁过渡带的地表温度和近地层大气温度很高, 和戈壁的地表温度接近;在多数晴天夜晚, 绿洲-戈壁过渡带的地表温度和近地层大气温度要低于戈壁的值.总辐射, 反射辐射和地表长波辐射的值都很接近荒漠戈壁的值, 日积分通量分别为24.48, 6.1, 41.42 MJ*m+-2*d.绿洲-戈壁过渡带的感热、潜热和地表热通量的日积分值分别为6.58, 1.60和0.38 MJ*m+-2*d.同时, 在绿洲-戈壁过渡带有较强的水平湍流输送. 相似文献
17.
新疆东部黑戈壁作为气候恶劣、人迹罕至的生态脆弱区，具有丰富的太阳能资源。利用红柳河陆气相互作用观测站2019年4、7、9月观测资料，分析东疆黑戈壁地表辐射及能量收支演变特征。结果表明：（1）地表辐射及能量收支各分量日变化均为单峰型。就不同季节而言，太阳总辐射和净辐射为夏季>春季>秋季，反射短波辐射为春季>夏季>秋季，地表和大气长波辐射为夏季>秋季>春季。（2）能量收支各分量季节变化明显，感热通量为春季>夏季>秋季，潜热通量为夏季>秋季>春季，地表土壤热通量为秋季>夏季>春季；能量分配在不同季节均以感热为主，地表土壤热通量次之，潜热通量极其微弱。（3）地表反照率日变化均为“U”型，在不同季节表现为春季>秋季>夏季，依次为0.29、0.27、0.26。东疆黑戈壁地表反照率整体较高，这是下垫面为黑色砾石所致。 相似文献
18.
I. Foyo-Moreno I. Alados F. J. Olmo J. Vida L. Alados-Arboledas 《Theoretical and Applied Climatology》2001,68(1-2):41-50
Summary Knowledge of ultraviolet radiation is necessary in different applications, in the absence of measurements, this radiometric
flux must be estimated from available parameters. To compute this flux under all sky conditions one must consider the influence
of clouds. Clouds are the largest modulators of the solar radiative flux reaching the Earth’s surface. The amount and type
of cloud cover prevailing at a given time and location largely determines the amount and type of solar radiation received
at the Earth’s surface. This cloud radiative effect is different for the different solar spectral bands. In this work, we
analyse the cloud radiative effect over ultraviolet radiation (290–385 nm). This could be done by defining a cloud modification
Factor. We have developed such cloud modification Factor considering two different types of clouds. The efficiency of the
cloud radiative effect scheme has been tested in combination with a cloudless sky empirical model using independent data sets.
The performance of the model has been tested in relation to its predictive capability of global ultraviolet radiation. For
this purpose, data recorded at two radiometric stations are used. The first one is located at the University of Almería, a
seashore location (36.83° N, 2.41° W, 20 m a.m.s.l.), while the second one is located at Granada (37.18° N, 3.58° W, 660 m
a.m.s.l.), an inland location. The database includes hourly values of the relevant variables that cover the years 1993–94
in Almería and 1994–95 in Granada. Cloud cover information provided by the Spanish Meteorological Service has been include
to compute the clouds radiative effect. After our study, it appears that the combination of an appropriate cloudless sky model
with the cloud modification Factor scheme provides estimates of ultraviolet radiation with mean bias deviation of about 5%
that is close to experimental errors. Comparisons with similar formulations of the cloud radiative effect over the whole solar
spectrum provides evidence for the spectral dependency of the cloud radiative effect.
Received November 15, 1999 Revised September 11, 2000 相似文献
19.
A physically-based solar radiation transmission model and a slope energy budget model were available which used climatic observations, averaged over 10-deg north-south latitude bands. This made possible the systematic examination of the diurnally changing energy budget components of net radiation, conduction, sensible, and latent heat flux occurring at all slope angles (0 to 90 deg) and slope directions (south-, west-, and north-facing). The present analysis utilized two contrasting landscapes along a latitudinal transect of the east coast of the Americas (northern hemisphere). Among the results, the maximum net radiation for all slope angles and directions occurred at noon on a 40-deg, south-facing slope for latitude 60. Generally, latent and sensible heat fluxes were similar in trend and magnitude between latitudes 0 and 35. Poleward, sensible heat flux increased with advancing latitude at the expense of latent heat flux. A great diversity in net radiation, sensible, and latent heat flux was obtained between different slopes and their orientation at a paniculate latitude. In addition to hourly rates of the energy budget components, daily positive sums of net radiation, sensible, and latent heat flux were examined. It is assumed that the portrayed patterns are general enough to add to our increasing understanding of the contrasts possible in a real-world north-south transect. 相似文献
20.
Simulation of the Bare Soil Surface Energy Balance at the Tongyu Reference Site in Semiarid Area of North China 
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下载免费PDF全文 ZHANG Xia 《大气和海洋科学快报》2010,3(6):330-335
The performance of a 1-D soil model in a semiarid area of North China was investigated using observational data from a cropland station at the Tongyu reference site of the Coordinated Enhanced Observing Period (CEOP) during the non-growing period, when the ground surface was covered with bare soil. Comparisons between simulated and observed soil surface energy balance components as well as soil temperatures and water contents were conducted to validate the soil model. Results show that the soil model could produce good simulations of soil surface temperature, net radiation flux and sensible heat flux against observed values with the RMSE of 1.54oC, 7.71 W m-2 and 27.79 W m-2, respectively. The simulated volumetric soil water content is close to the observed values at various depths with the maximal difference between them being 0.03. Simulated latent heat and ground heat fluxes have relatively lower errors in relative to net radiation and sensible heat flux. In conclusion, the soil model has good capacity to simulate the bare soil surface energy balance at the Tongyu cropland station and needs to be further tested in longer period and at more sites in semiarid areas. 相似文献