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1.
卷云与水云的短波透射与反射特性   总被引:8,自引:1,他引:7  
利用矩阵算法计算了对不同太阳天顶角下不同光学厚度的卷云与水云,在4π空间内0~360o的不同方位与0~90o不同天顶角下的波长为1.39 μm太阳短波波段的透射与反射,其天顶角间隔为5.6o,方位角间隔为5.0o。可以看出两种云透射和反射辐射的差别及它们随着光学厚度变化而变化的情况。同时,将其与波长为0.55 μm的可见光波段的透射和反射进行了比较。  相似文献   

2.
西藏当雄地基紫外线指数观测研究   总被引:1,自引:1,他引:0       下载免费PDF全文
基于西藏当雄2009年9月—2011年8月地基紫外线指数 (UVI) 观测,结合TUV辐射传输模式分析, 该文检验太阳天顶角、云、臭氧、积雪和气溶胶对UVI的影响。结果显示,影响地面UVI主要因素是太阳天顶角和云。晴天地面UVI可简单用太阳天顶角拟合函数表征;地面UVI的云调制因子总体上随云量增加呈下降趋势,但间隙性、未遮蔽日面的云可增强太阳散射辐射,使云调制因子值平均增加约3%~6%,个别情形达40%。臭氧低谷使当雄UVI比同纬度平原地区增加约12%;冬季短期、浅层积雪使UVI增加16%或更低,也低于模式模拟值 (23%);气溶胶 (光学厚度为0.02~0.1) 对UVI衰减低于3%。因臭氧低谷导致青藏高原臭氧南北分布的差异,相同太阳天顶角下拉萨 (海拔为3650 m) UVI较瓦里关 (海拔为3810 m) 偏高7%~10%。与卫星产品比较表明:OMI卫星UVI产品在当雄、沱沱河、瓦里关和拉萨较地基测值总体偏高65%以上,而晴天则平均分别偏高8.6%,13%,9%和50%。云、地基与卫星像元地理位置差异应是卫星UVI产品偏高的原因。当雄地基UVI测值大于14时,卫星UVI产品反而低3%应与间隙性云有效增强了地面辐射有关。  相似文献   

3.
利用2007—2009年热带降雨测量卫星(TRMM)的微波成像仪(TMI)观测到的亮温资料,计算9个通道(10、19、37、85 GHz的水平和垂直极化通道及21 GHz的垂直极化通道)的亮温和极化修正温度(PCT)在不同范围内的最大值、最小值、平均值和区域阈值与热带气旋强度之间的关系。结果表明:亮温信息可较好地反映热带气旋的强度,单个参数与热带气旋最大风速的相关性最好可达到0.83,线性拟合的均方根误差接近业务误差;低频通道的亮温相对于高频通道可更好地估计海上热带气旋强度;位于台风中心0.5°~1.5°度范围之间的亮温与气旋强度的相关性较好,圆形区域的相关性好于圆环区域;对于位于海上的热带气旋,区域亮温的最小值与热带气旋强度的关系最好;低频通道(除10 GHz外),阈值位于260~280 K区间的亮温与热带气旋强度的相关性较好。  相似文献   

4.
【目的】为了研究全球降水测量计划(GPM)综合多卫星检索降水产品(IMERG)在浙江省的适用性。【方法】以浙江省为研究区域,基于浙江省自动观测站降水数据,利用相关系数、均方根误差、相对偏差、分类指数统计法分别从年尺度、季尺度、月尺度、日尺度以及小时尺度GPM在浙江省的适用性。【结果】(1)春、秋、冬季的GPM和自动站对应效果远好于夏季,月尺度、日尺度、小时尺度下GPM和自动站降水数据对应效果较好,但整体上存在高值区略低估、低值区略高估现象;(2)年尺度与季尺度下GPM与自动站降水平均值的变化趋势一致,但GPM降水平均值较高,其中秋季表现最好;(3)年、月、日3个尺度下,尺度越精细化,相关系数越高、相对偏差越小,均方根误差越小;小时、日、月3个尺度下,降水阈值越低,产品尺度越粗糙,估测能力越高;降水阈值越低,产品尺度越精细,误报降水的比例越低;降水阈值越低,综合探测能力越高;(4)在小时尺度下,在0.5~1 mm·h-1区间,GPM虽然对降水事件略有高估,但拟合效果较好。【结论】综合来看,GPM日尺度降水数据产品精度在浙江省有较大应用潜力。  相似文献   

5.
为评估全球降水观测(GPM)卫星降水数据在广东地区的适用性,利用广东省86个国家地面站点实测降水数据,选用5个评价指标从降水误差、季节平均降水量等方面进行精度验证。结果表明:(1)GPM卫星降水数据与站点实测数据相关性随时间尺度增加呈递增趋势,探测能力在月尺度上表现较好。(2)GPM卫星降水数据在季节尺度上对平均降水量有一定的表征能力,但季节间有明显差异,在夏季表现较差。(3) GPM降水数据受气候、地理位置和地形等因素影响较大,降水精度易受影响。  相似文献   

6.
卫星微波仪器接收的来自地气系统的被动热辐射与主动传感器发射的信号相混合,被称为无线电频率干扰 (RFI),在主动及被动微波遥感探测领域已成为越来越严重的问题。海洋表面反射的静止通讯、电视卫星下发信号是干扰海洋上星载被动微波辐射计观测的主要来源。该文以先进的微波扫描辐射计AMSR-E为例,采用双主成分分析方法对美国陆地上大面积水体、附近洋面和中国海岸线附近的RFI进行识别,研究表明:美国附近洋面区域星载微波辐射计18.7 GHz通道观测主要受静止电视卫星DirecTV的干扰,由于海表反射引起的RFI非常依赖于静止卫星和星载被动仪器的相对几何位置,只有当闪烁角θ(观测视场镜面反射的静止电视卫星信号方向与视场到星载仪器方向之间的夹角) 较小时卫星观测易受到污染。美国海洋区域较强RFI分布在五大湖区域,离内陆越近RFI越强,东西海岸RFI较强,而整个南海岸干扰相对较弱。中国海岸线附近AMSR-E 6.925 GHz通道观测受RFI影响,而18.7 GHz通道观测未受到干扰。  相似文献   

7.
由于缺乏庞大的水文测量系统,难于得到地表能量平衡各分量的准确空间平均值.本文旨在建立一种利用遥感方法估测不同作物冠层状况下地表能量平衡分量之一的土壤热通量的方法,以用于区域地表能量平衡研究.在亚利桑那州靠近菲尼克斯城的Maricopa农业中心,连续几天测定了裸地、苜蓿地及棉田的净辐射(Rn)和土壤热通量(G),并利用多波段辐射仪测得地面反射率.结果表明:中午土壤热通量和净辐射的比(G/Rn)与简单比及标准化差植被指数呈线性相关.棉田的G/Rn估算值实际上与不同太阳天顶角和方位角得到的光谱资料所引起的植被指数变化没什么关系,因此多波段光谱资料可为区域能量平衡研究提供一种能准确计算土壤热通量区域平均值的方法.  相似文献   

8.
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   

9.
以黄河源区水文循环过程为主要研究对象,应用TRMM卫星和GPM卫星的日降水产品(TMPA3B42和IMERG-Final)驱动流域分布式水文模型SWAT,将结果进行比较分析,评估了新型卫星降水在黄河源区的适用性及其模拟潜力。研究表明:(1)对于大尺度流域而言,同时对多个子流域进行参数的敏感性分析及率定的结果不适用于每一个站点。因此,本文采用对每个水文站点所对应的子流域依次进行敏感性分析与验证的方式进行订正,最终得到验证期内3个站点径流模拟结果的纳什效率系数均在0.50以上,决定系数都在0.60以上。(2)从模拟结果来看,IMERG-Final产品的模拟结果要优于TMPA3B42产品。两种卫星降水产品均能模拟出黄河源区月径流变化的主要趋势,但均表现为对于径流峰值的模拟偏高。新型卫星产品(GPM)较前任TRMM卫星产品的精度确实有提高,且具备一定的模拟潜力,但对于高海拔地区的模拟能力有待提高,需要进一步订正。  相似文献   

10.
狄迪  周镕连  赖睿泽 《气象学报》2022,80(4):632-642
新一代静止气象卫星成像仪具有高时、空分辨率的优势,成像仪的云观测资料被广泛应用于气象领域的各项研究中。由于卫星的观测方式和地球曲率导致其存在视场偏差,与其他资料联合应用时需要考虑其影响。针对风云四号A星成像仪的视差问题,首先使用模拟的云顶高度和实际的卫星天顶角进行敏感性分析,结果证实云顶高度越高或者卫星天顶角越大则视差越大, 尤其对具有更高空间分辨率的成像仪,视差影响更需要被重视。随即分别使用CALIPSO云层数据和3套台风最佳路径集来检验视差订正前、后的多通道扫描辐射成像仪(AGRI)云检测产品和台风中心定位的精度,结果证明所用的视差订正方法是有效的,并指出在静止气象卫星资料的精确定量应用中,视差不可忽视。   相似文献   

11.
先进微波辐射计(AMSR-E)的低频特性使其更容易受到无线电频率干扰(RFI),本文首先对比了谱差法和双主成分分析(Double Principal Component Analysis,DPCA)方法这两种RFI识别算法的差异,验证了DPCA方法的适用性,然后选用DPCA方法对2002年9月—2011年9月AMSR-E陆面升轨亮温月平均数据中的RFI进行识别,并分析其多年变化特征。DPCA方法可以有效地识别出AMSR-E全球范围内陆地亮温数据中的RFI分布情况。识别结果显示:1)C波段中的RFI主要分布在美国、东亚及印度—阿拉伯半岛地区;X波段主要分布在欧洲及东亚地区。2)各区域的RFI空间位置及强度随时间会发生变化,其原因可能是由于基础设施及使用无线电频谱的变化造成。3)不同区域月平均亮温数据中识别出的RFI信号数量存在季节变化,并且C波段中识别出的RFI数量随时间减少,X波段中随时间增加。  相似文献   

12.
基于2014年8月1—16日AMSR-2的观测资料,采用谱差法重点对东亚陆地低频7.3 GHz的无线电频率干扰(RFI)进行识别与分析。研究发现,东亚地区7.3 GHz通道观测存在无线电频率干扰,其中韩国京畿道、大邱市,孟加拉国,越南及柬埔寨东南部地区的干扰源是稳定、持续的地面主动源。日本地区7.3 GHz通道RFI仅出现在AMSR-2升轨观测上,而降轨观测则几乎不受干扰,且RFI污染区出现的位置与强度随时间及辐射计扫描角度周期性变化,探究其污染源,发现主要来自地面反射的静止通信/电视卫星信号对星载微波被动传感器观测的干扰。  相似文献   

13.
用于空间对地遥感的一个参数化辐射传输计算模式   总被引:4,自引:1,他引:3  
邱金桓 《大气科学》1998,22(4):649-658
一个足够精度的参数化向上亮度模式对空间对地遥感的大气订正应用是很有意义的。依据向上天空亮度对大气散射相函数、光学厚度、太阳天顶角、空间方位和天顶角等有关参数的依赖特性,基于大量的天空亮度数值模拟计算资料,本文发展了一个关于向上天空亮度的参数化模式。39440组的数值模拟对比资料表明,在气溶胶光学厚度#Aτt≤1,太阳天顶角小于72°,μ≤0.432 (天顶角小于65°)以及无云的条件下,由现在的参数化的模式所计算的向上亮度的误差一般小于6%。地表反射率越大,参数化模式的精度越高。参数化模式的精度一般随着光学厚度和太阳天顶角的增大而变差。  相似文献   

14.
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   

15.
Summary The dependence of the albedo on illumination direction is analyzed by constructing a canopy model in which the individual leaves are planar, Lambertian reflectors. Leaf transmission is treated separately, and is assumed to be proportional to the cosine of the zenith angle of the leaf normal. Effects of shading and obscuration are formulated assuming random distribution of the leaves with respect to the viewing and illumination directions. Variants of the model with different azimuthal leaf distributions are created and discussed as explicit expressions of the viewing/illumination geometry and the canopy characteristics.The canopy spectral single-scattering albedo factors, which are the conditional probabilities of a photon escaping from the canopy after a first reflection or a first transmission, are obtained by numerical integration over a hemisphere of the bidirectional reflectance and transmittance factors. Our analysis identifies the ratio of the projection of leaf area on the vertical plane perpendicular to the principal plane to that on a horizontal plane as the parameter that controls the dependence of the albedo on the solar zenith angle. The albedo factor due to the leaf transmittance generally increases with the zenith angle of illuminating beam more sharply than that due to the leaf reflectance.Model variants with various azimuthal distributions are compared with measured albedo of soybeans. Second and higher order scatterings are accounted for in a simplified way. The degree to which a model variant fits the measured albedo and its change with the solar zenith angle depends both on the leaf inclination angleand the azimuthal distribution of the leaf area.With 6 Figures  相似文献   

16.
The authors analyzed the retrieval sensitivity of tropospheric ozone using simulated the Global Ozone Monitoring Experiment-2 (GOME-2) measurements. The retrieval sensitivity was evaluated by the degree of free- dom for signal (DFS). The combination of the ultraviolet (UV), UV polarization (UVPOL), and visible (VIS) bands enhances DFS of tropospheric ozone and improves the vertical resolution of the retrieved ozone profile. UVPOL reduces the dependence on solar zenith angle, mainly in- creases the sensitivity in upper troposphere. Polarization increased the DFS by 20% on the eastern side of the GOME-2 orbit, with little improvement on the western side because the increase in DFS due to polarization is depend- ent on the relative azimuth angle. The inclusion of the visi- ble band reduces significantly the dependence on viewing geometry, and mainly increases the DFS in the lower tro- posphere (0-6 kin) by a factor of two. It was possible to retrieve several independent pieces of tropospheric ozone information from GOME-2 UV/UVPOL/VIS measure- ments, especially in the lower troposphere.  相似文献   

17.
本文发展了一个从宽带水平面太阳直接辐射日曝辐量 (总辐射与散射辐射日曝辐量之差) 反演光谱大气气溶胶光学厚度的方法, 包括建立一个 “等效” 的瞬时太阳天顶角模型, 并提出了一个基于气溶胶标高的云影响甄别方法。对该反演方法的数值模拟和误差分析表明: “等效” 瞬时太阳天顶角模型的不稳定性引起的光学厚度反演误差平均为3.66%; 光学厚度日变化对一段较长时间的平均光学厚度的影响不显著; 订正造成的散射辐射误差≤20%时, 光学厚度平均偏差≤4%。通过与AERONET产品的比对验证表明: 本文发展的光学厚度反演方法和云影响甄别方法都是有效的; 晴空反演的0.75 μm光学厚度与AERONET的相关系数超过0.95, 平均误差约0.02; 云甄别方法计算的季节和年平均光学厚度与AERONET具有较好的一致性。  相似文献   

18.
Surface erythemal UV radiation is mainly affected by total column ozone, aerosols, clouds, and solar zenith angle. The effect of ozone on the surface UV radiation has been explored many times in the previous studies due to the decrease of ozone layer. In this study, we calculated the effect of aerosols on the surface UV radiation as well as that of ozone using data acquired from Ozone Monitoring Instrument (OMI). First, ozone, aerosol optical depth (AOD), and surface erythemal UVB radiation measured from satellite are compared with those from ground measurements. The results showed that the comparison for ozone was good with r 2 of 0.92. For aerosol, there was difference between satellite measurements and surface measurements due to the insufficient information on aerosol in the retrieval algorithm. The r 2 for surface erythemal UV radiation was high (~0.94) but satellite measurements showed about 30% larger values than surface measurements on average by not considering the effect of absorbing aerosols in the retrieval process from satellite measurements. Radiative amplification factor (RAF) is used to access the effect of ozone and aerosol quantitatively. RAF for ozone was 0.97~1.49 with solar zenith angle. To evaluate the effect of aerosol on the surface UV radiation, only clear-sky pixel data were used and solar zenith angle and total column amount of ozone were fixed. Also, RAF for aerosol was assessed according to the single scattering albedo (SSA) of aerosols. The results showed that RAF for aerosol with smaller SSA (< 0.90) was larger than that for with larger SSA (> 0.90). The RAF for aerosol was 0.09~0.22 for the given conditions which was relatively small compared to that for ozone. However, considering the fact that aerosol optical depth can change largely in time and space while the total column amount of ozone does not change very much, it needs to include the effect of aerosol to predict the variations of surface UV radiation more correctly.  相似文献   

19.
本文针对南京溧水S波段双偏振多普勒天气雷达获取的回波I/Q信号,采用FFT算法处理水平和垂直通道I/Q数据,分别得到水平和垂直通道回波的强度、速度值,定性分析了两通道回波强度、速度数据差异,引入平均差及均方根误差参数做定量分析。对比结果表明:两通道I/Q数据处理得到的回波层次分布基本一致;两通道速度数据差异较小,强度数据差异较大。以水平通道回波数据为基准,当回波强度小于16 dBz时,水平通道强度偏小,这可能是由云系边缘较小的针状冰晶所致;当回波强度大于32 dBz时,水平通道强度值偏大,且随回波强度的增加两通道强度差值增大,这反映了强降水中大粒子较多,而粒子越大,降落过程中扁平程度越大;两通道回波强度的差值与回波强度大小呈现一定相关性,这可能反映了单偏振天气雷达在定量测量降水中精度不高,通过双偏振雷达联合利用两通道数据有望改善雷达定量测量降水精度,提升雷达定量估测降水能力。  相似文献   

20.
Summary An angular dependence model (ADM) is needed to convert radiance measurements into fluxes. This paper provides an overview on the progress and issues related to the angular correction of radiation data at the top-of-the-atmosphere (TOA), followed by an investigation on the performance of the Earth Radiation Budget Experiment (ERBE) ADMs in the Arctic during summer. The variation of inferred albedo with viewing geometry indicates the merit of an ADM. The ERBE ADM for land does well as it leads to near constant albedos for given solar zenith angles. The ADM for snow/ice is least satisfactory when applied to the Arctic in summer. The performance of the ocean ADM is acceptable except at large solar zenith angles for which albedo increases with viewing zenith angle. Significant and systematic variation of albedo with viewing angle and relative azimuth angle are manifest when the overcast ERBE ADM is applied to over-cast-over-snow/ice scenes. A methodology for correcting ERBE ADMs was proposed by normalizing the anisotropic factor over bins containing sufficient measurements.With 6 Figures  相似文献   

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