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1.
FY-1C遥感器可见近红外各通道在轨辐射定标 总被引：13，自引：0，他引：13
文中通过 1999年 7月利用敦煌辐射定标场和反射率基法对FY -1C气象卫星遥感器可见 -近红外通道进行的第一次在轨辐射定标试验 ,研究和试验了卫星遥感器的在轨辐射定标方法、同步观测方法和辐射传输计算算法及其软件开发 ,有 7个通道的绝对辐射定标系数 (或称为增益和偏离量 )被获得。经过误差分析 ,认为本次定标的不确定度小于 7%。定标获得的 7个通道定标系数与该卫星发射前定标结果比较 ,其中 5个通道 (通道 1,2 ,7,8,10 )结果比较接近 ,另两个通道 (通道 6,9)由于发射前定标误差较大致使二者有一定差别。另外 ,通过 2 0 0 0年 9月份对FY -1C卫星进行的第二次辐射定标试验 ,使该卫星在轨 1a多来的运行状态得到了定量监测 ,本次定标与1999年 7月的定标结果比较 ,发现可见 -近红外各通道性能均有程度不同的衰减 ,尤其是通道 1,7,8性能衰减分别为 35% ,2 8% ,2 2 % ,而通道 2 ,6,9,10性能衰减较小 (为 10 %左右 )。 相似文献
2.
VICARIOUS RADIOMETRIC CALIBRATION OF SATELLITE FY-ID SENSORS AT VISIBLE AND NEAR INFRARED CHANNELS 
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下载免费PDF全文 ZHANG Yuxiang QIU Kangmu HU Xiuqing RONG Zhiguo ZHANG Lijun 《Acta Meteorologica Sinica》2004,18(4):505-516
For the problem of in-flight test site radiometric calibration for the FY-1D Meteorological Satellite onboard sensor's visible and near infrared channels,this paper described the calibration method,satellite-ground synchronous observation data acquired at China Dunhuang Calibration Test Site,parameter derivation and radiative transfer computation during the calibration,and the calibration result analysis.At FY-1D seven channels (with central wavelength at Channels 1:630 nm,2:865 nm;6:1610 nm;7:455 nm,8:505 nm;9:555 nm;10:932 nm),calibration coefficients obtained during the ground site calibration were compared with that respectively of prelaunch calibration.It is demonstrated that results of FY-1D onboard two sensors' (A and B) at channels 1,2,6 and 10 were close to pre-calibration,and the absolute difference of Gobi desert reflectance computed using test site and pre-launch calibration coefficients was no more than 2%. At other channels,large pre-launch calibration errors resulted in a poor consistency between the test site and pre-launch calibration.The errors can be corrected by the test site calibration results. Based on a rough estimation,the overall error of the calibration was about 6%. The paper also presented the in-flight vicarious calibration at the visible and near infrared channels of FY-1C sensor A which was launched in 1999 and has been put into operational mode since 2002.The results exhibit that FY-1C sensor's response has 23% attenuation at Channels 7 and 8,while only minor degradation at the other channels was found. During the mission,calibrations were also conducted at NOAA-17's Channels 1 and 2 (1:430-830 nm,2:500-1072 nm).A very good consistency has been achieved between the test site and pre-launched calibration results. 相似文献
3.
利用2007年8月在策勒用ASDFR光谱辐射计探测的数据,以及国家卫星中心在敦煌辐射校正场的观测资料,运用参考板野外反射率因子修正法计算了地表反射率,并对比分析了策勒考察场和敦煌辐射校正场地理条件及地表反射率的特点。结果表明：在地理条件上,策勒考察场交通便利,晴空日数多,恢复能力好,不受人为因素影响,若作为辐射校正场具有持久性;策勒辐射考察场中心区平均反射率在28．9％左右,基本位于卫星遥感传感器的中心段,可以满足大多数卫星遥感传感器的辐射校正;地表反射率最大在2100nm附近,约为0.38,平均偏差约1.3％。比较得出,策勒考察场地表均匀性较好,其反射率较敦煌的略高,而偏差略低。所以,策勒考察场的地理条件和地表反射比符合作为辐射校正场的条件,且与敦煌校正场相比具有一定的优势。 相似文献
4.
1999年6月28日~7月19日在敦煌场, 7月25日~7月31日在青海湖水面场进行了一次大规模综合野外测量试验, 其中采用3台先进的法国CIMEL太阳辐射计对两个场地大气光学特性进行了系统全面测量, 获得大量晴空天气条件下的大气光学数据。利用Langley法处理气溶胶通道数据得到气溶胶光学厚度及其光谱变化。测量结果显示550 nm波长平均气溶胶光学厚度分别为0.12、0.18, 由气溶胶光学厚度的波长变化得到气溶胶Junge参数分别为2.6、3.0, 并与几种典型气溶胶类型比较。结果表明两地在晴空天气里, 气溶胶含量较小, 符合遥感卫星传感器辐射定标的大气条件。 相似文献
5.
比较分析了2017年南极中山站3种仪器测量地面太阳紫外B（UVB）波段和紫外A（UVA）波段的辐照度。以Brewer光谱仪测值为参考,国产宽波段FSUVB日射表在UVB（波段280~315 nm）的辐照度相对误差为（55±75）%,误差随大气臭氧总量的增加呈上升趋势,但在南极“臭氧洞”期间偏低。Yankee UVB宽波段日射表在UVB（波段280~320 nm）的辐照度相对误差为（-31±22）%;国产宽波段FSUVA日射表在UVA（波段315~400 nm）的辐照度相对误差为（23±5.9）%。太阳天顶角低于80°的晴天以Tropospheric Ultraviolet Visible（TUV）辐射模式计算结果为参考时,FSUVB,Yankee UVB和FSUVA辐照度的平均相对误差分别为（30±37）%,（-22±19）%和（27±6.4）%,而Brewer相对误差未超过3.5%。国产宽波段UV日射表测值偏高,反映出波长较长的杂散光对太阳辐照度测值影响明显。 相似文献
6.
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
7.
该研究是加拿大Saskatchewan Scott农作物轮作系统(ACS)研究的一部分。研究始于1994年,历时18a,评价9个可耕种农作物产量系统的可靠性。由3种处理水平(organic,reduced,high)和3种作物多样性水平(low,diversified annual grains,diversified annual perennials)结合而产生的9个农作物产量系统,被用于监测和评价加拿大牧场不同处理和不同作物种植轮作下可耕种农作物的产量。在2003年生长季共收集了3次叶面积指数和光谱反射率的数据:生长季前期(6月)、生长季旺盛期(7月)、生长季后期(8月)。叶面积指数是由LAI-2000植物冠层分析仪监测的,光谱测量是由覆盖了350-2500 nm波长范围共2215个波段的ADS便携式高光谱仪完成的。结果显示,光学测量可以用于监测农作物生长状况的差异。从生长季的早期到中期,光谱和叶面积指数在不同处理下有显著差异。7月中期是用遥感资料监测农作物长势的最佳季节;红光波段与近红外波段反射率的比值和基于这两个波段构造的归一化植被指数,是检测农作物长势的最佳植被指数。 相似文献
8.
对大面积水体进行水质遥感监测是比较典型的水体环境监测手段。该文利用地物光谱仪测定了巢湖水面的光谱反射率, 收集了相应时间的MODIS数据, 经过预处理之后, 首先分析了巢湖水面光谱特征, 并对实测水体反射率与实测叶绿素a之间的关系进行统计拟合计算。在经过MODIS大气校正后, 得到1~7通道的地表反射率。利用大气校正后的EOS/MODIS数据, 选择最佳通道组合, 定义了叶绿素a指数IChla, 建立了MODIS巢湖叶绿素a浓度的反演模型, 检验得到相关系数为0.5079。 相似文献
9.
由大气顶射出太阳辐射的形式解出发,结合球形粒子的米散射理论,由反射太阳光谱推导获得了反演整层大气气溶胶粒子体积谱分布的权重函数。在权重函数特征分析的基础上,根据一个简单的线性反演算法,利用大气辐射传输计算模拟的大气顶反射太阳光谱,反演获得了不同气溶胶浓度和复折射率条件下的气溶胶粒子体积谱。结果表明,初步建立了一套自洽的大气气溶胶体积谱分布的反演方法。通过米散射计算获得的反演参数考虑了波长对粒子半径的权重特征,使气溶胶体积谱的反演具有了明确的物理依据;同目前常用的查算表方法相比,简化了反演方案中参数化的复杂程度。 相似文献
10.
Retrieval of aerosol optical properties over a vegetation surface using multi-angular,multi-spectral,and polarized data 总被引：1，自引：0，他引：1
An algorithm to retrieve aerosol optical properties using multi-angular,multi-spectral,and polarized data without a priori knowledge of the land surface was developed.In the algorithm,the surface polarized reflectance was estimated by eliminating the atmospheric scattering from measured polarized reflectance at 1640 nm.A lookup table （LUT） and an iterative method were adopted in the algorithm to retrieve the aerosol optical thickness （AOT,at 665 nm） and the （A）ngstr（o）m exponent （computed between the AOTs at 665 and 865 nm）.Experiments were performed in Tianjin to verify the algorithm.Data were provided by a newly developed airborne instrument,the Advanced Atmosphere Multi-angle Polarization Radiometer （AMPR）.The AMPR measurements over the target field agreed well with the nearby ground-based sun photometer.An algorithm based on Research Scanning Polarimeter （RSP） measurements was introduced to validate the observational measurements along a flight path over Tianjin.The retrievals were consistent between the two algorithms.The AMPR algorithm shows potential in retrieving aerosol optical properties over a vegetation surface. 相似文献
11.
测站附近微环境条件对地面气温观测记录的影响目前还不清楚。本文对2010年漠河国家基准气候站地面观测对比试验数据进行了分析,得到如下结论:(1)年平均地面气温近障碍物点低于标准观测场内,但1、6月的月平均气温近障碍物点偏高;(2)06:00—17:00和21:00,近障碍物地点的气温偏低;18:00至次日05:00(除21:00),近障碍物点气温偏高;(3)春季各时次近障碍物点地面气温均偏低;夏季06:00—17:00近障碍物点气温偏低,18:00至次日05:00相反;秋季仅01:00、03:00、19:00、23:00近障碍物点气温偏高,其他时次相反;冬季07:00—19:00近障碍物点气温偏低,20:00至次日06:00相反。冷季近障碍物点气温偏低;暖季昼间近障碍物点气温偏低,夜间相反;(4)日最高、最低气温出现时间不同地点大体相同,最高气温近障碍物点偏低,最低气温近障碍物点偏高,但最高气温偏低绝对值大于最低气温偏高绝对值;(5)有雾情况下近障碍物地点的气温偏高几率大;雨雪多云天气近障碍物地点气温均偏低;晴朗的白天近障碍物地点的气温偏低,有风天气更明显;而晴朗的夜间近障碍物地点气温偏高,无风天气更明显;晴朗天气条件下,无风时近障碍物地点与观测场内气温差值大于有风时。结果表明,地面气温观测记录对台站观测场附近微环境改变十分敏感,微环境条件的变化将导致地面气温观测出现明显不连续性,对气候变化分析产生影响。 相似文献
12.
By W. VON HOYNINGEN-HUENE T. DINTER A. A. KOKHANOVSKY J. P. BURROWS M. WENDISCH E. BIERWIRTH D. MÜLLER M. DIOURI 《Tellus. Series B, Chemical and physical meteorology》2009,61(1):206-215
Main optical characteristics of desert dust, such as phase function and single scattering albedo, have been derived from combinations of sun-/sky-radiometer and satellite measurements during the SAMUM experiment (10 May–10 June 2006) at the site Porte au Sahara (30.237°N, 5.607°W) in South Morocco. Scattering phase functions have been retrieved using combined data of spectral aerosol optical thickness (AOT) and spectral sky brightness in the almucantar, considering non-spherical light scattering. Intercomparisons of modelled top-of-atmosphere (TOA) reflectance with satellite observations of the Medium Resolution Imaging Spectrometer (MERIS) and Scanning Imaging Absorption Spectrometer for Atmospheric Chartography () instrument have been used for the estimation of spectral single scattering albedo. For the radiative transfer calculations scattering phase functions and AOT from ground-based observations have been used. The spectral single scattering albedo ranges from 0.93 in the blue to 0.98 at 753 nm. 相似文献
13.
Summary Surface reflectance factors from bare field soil were measured to determine the relationship between surface soil water content and spectral reflectance. Reflectance in the six reflective Thematic Mapper (TM) bands plus a 1.15 to 1.30 µm bandpass (referred to as MMR 5) was measured using a groundbased radiometer across a soil water gradient provided by a line source sprinkler system. A spectral index of soil brightness (Brightness) derived using the Gram-Schmidt process and utilizing reflectance information was calculated for each band and for combinations of bands. The results of this study show that TM band 7 (2.05–2.30 µm) provided improved estimates of surface soil water content (0–0.5 cm depth) over estimates using reflectance information from all seven bands. Good correlations were also found between band ratio spectral indices of TM 5 (1.55–1.75 µm) / TM 7, MMR 5/TM 7, and MMR 5/TM 5 and surface soil water content. Results indicate that surface reflectance factors within bandpasses that partially overlap water absorption regions, such as TM 7, are most highly correlated with surface soil moisture. Band ratios utilizing a bandpass partially overlapping a water absorption region such as TM 7 and a non-water-absorbing bandpass such as MMR 5 yield close correlations with surface soil water content.Contribution from the Arizona Agricultural Experiment Station, Tucson, AZ 85721. Journal Paper No. 7040.With 6 Figures 相似文献
14.
Yuanzhi Zhang Hongtao Duan Hongyan Xi Zhaojun Huang JinYeu Tsou Tingchen Jiang 《大气与海洋》2018,56(4):277-288
AbstractAquatic plants and lake bottoms in optically shallow waters (OSWs) wield great influence on reflectance spectra, resulting in the inapplicability of most existing bio-optical models for water colour remote sensing in lakes. Based on radiative transfer theory and measured spectra from a campaign for Lake Taihu in October 2008, absorption and backscattering coefficients were used to simulate the remote-sensing reflectance, which are considered to be reliable if matched to their measured counterparts. Several cases of measured spectra at different depths, Secchi disk depth transparency, and aquatic plant height and coverage were analyzed thoroughly for spectral properties. The contribution of aquatic plants was evaluated and compared with the measured and simulated remote-sensing reflectance values. This is helpful for removing the influence of aquatic plants and lake bottoms from the spectra and for constructing an improved chlorophyll a retrieval model for OSWs, such as that for Lake Taihu, China. 相似文献
15.
利用欧洲中期数值预报中心的ERA40再分析逐日的200 hPa风场资料,选取1958—1977年和1980—1999年各20年,对比分析了在全球变暖背景下前后两个时段热带大气季节内振荡(ISO)的特征及其变化。研究表明:近20 a来,原来在赤道中太平洋上活跃的ISO减弱,而在中印度洋、孟加拉湾地区ISO变得活跃;全球变暖背景下,ISO的强度变化幅度加大,表明ISO更加活跃,且季节变化明显,冬、春季强,夏、秋季弱;对流层上层的纬向风能量更集中于1—3波,ISO的频率有加大的趋势。还利用中国科学院大气物理研究所LASG发展的耦合气候系统模式FGOALS-1.0g中的控制试验及其二氧化碳浓度加倍试验结果,分别对应实测资料的前后20年进行对比分析。发现模式对ISO的空间结构模拟较好,但低估了ISO的强度;时空谱分析表明模式结果中包含有更多的纬向风的高频成分,由于能量的分散,导致对ISO活动强度的低估。但通过对模式的控制试验和温室气体增加试验结果的对比分析,发现耦合模式还是较好地反映出在全球变暖背景下ISO在中印度洋、孟加拉湾地区变得活跃、频率加大等变化特征。 相似文献
16.
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
17.
The ultraviolet (UV) spectra on cloudy days were compared to those on cloud free days to determine which part of the UV spectrum has the greatest enhancement due to the cloud compared to both corresponding measured clear sky spectra as well as other enhanced spectra. In this preliminary study, cloud enhanced UV spectra selected for maximum UVA enhancement compared to a clear sky UV spectrum at similar solar zenith angle (SZA) and ozone values, showed that the ratio of the two sets of spectral irradiances was approximately wavelength independent (approximately 1.1) above the cut-off wavelength of approximately 306 nm. Similarly, above 306 nm the average ratio of the spectral irradiances of a maximum UVB enhanced UV spectrum compared to a clear sky spectrum was 1.2 with maximum values generally above this average between 316 and 344 nm and generally below 1.2 above the wavelength of 344 nm. The UVA and UVB enhanced spectra were separated into five SZA ranges and the irradiance at each wavelength averaged for each range and compared to clear sky spectra in each of the ranges. Above approximately 306 nm, the ratios are wavelength independent for all SZA. However, with the exception of the SZA range centred on 20°, there is an increasing dependency with shorter wavelengths below the 306 nm. Also there appears to be two distinct groupings of the average irradiance ratios, corresponding to the SZA range centred on 20°, 37° and 49° (ratio of 1.2) and 32° and 42° (ratio 1.0), the latter cases suggesting that on average there is no enhancement for these SZA, except for wavelengths less than 306 nm. 相似文献
18.
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
19.
By C. TOLEDANO M. WIEGNER M. GARHAMMER M. SEEFELDNER J. GASTEIGER D. MÜLLER P. KOEPKE 《Tellus. Series B, Chemical and physical meteorology》2009,61(1):216-228
The aerosol optical depth (AOD) in the range 340–1550 nm was monitored at Ouarzazate (Morocco) during the Saharan Mineral Dust Experiment (SAMUM) experiment in May–June 2006. Two different sun photometers were used for this purpose. The mean AOD at 500 nm was 0.28, with a maximum of 0.83, and the mean Ångström exponent (AE) was 0.35. The aerosol content over the site changed alternatively from very low turbidity, associated to Atlantic air masses, to moderate dust load, associated to air masses arriving in the site from Algeria, Tunisia and Libya. The dusty conditions were predominant in the measurement period (78% of data), with AOD (500 nm) above 0.15 and AE below 0.4. The spectral features of the AOD under dusty conditions are discussed. Air mass back trajectory analysis is carried out to investigate the origin and height patterns of the dust loaded air masses. The advection of dust occurred mainly at atmospheric heights below 3000 m, where east flow is the predominant. At the 5000 m level, the air masses originate mainly over the Atlantic Ocean. Finally the Optical Properties of Aerosols and Clouds (OPAC) model is used to perform a set of simulations with different aerosol mixtures to illustrate the measured AOD and AE values under varying dust concentrations, and a brief comparison with other measurement sites is presented. 相似文献
20.
The relationship between the radiance ratio (radiance at wavelength 450 nm to 650 nm) and aerosol optical depth (AOD) is analyzed in this paper by numerical simulation and a "LUT" (look-up table) approach is then presented for the retrieval of AOD from the radiance ratio. In this LUT approach, the AOD retrieval error depends mainly on the assumption of aerosol types. From the preliminary simulation, a typical error of 15%–20% in AOD obtained from the radiance ratio is estimated, due to neglecting changes in... 相似文献