PSP总日射表灵敏度系数的热偏移订正方法

PSP总日射表在我国一直作为标准总日射表和质量优良的辐射仪器在使用,2006年以前还曾作为国家散射标准,在太阳辐射量值传递中测量标准散射辐射,通过成分和法计算标准总日射辐照度。总日射表的校准在晴天条件下进行,此时天空无云,由于热偏移为负值,导致对短波灵敏度系数被低估。2011年10月14日—11月15日在北京密云上甸子大气本底站进行了对比观测试验,通过对不同总日射表热偏移订正方法的试验与研究,进行了5种热偏移订正方法的比较。通过订正,在用于室外成分和法校准时,PSP表的灵敏度系数的准确度可提高1%,进而提高总辐射的测量准确度。     

总辐射表夜间零点偏移试验与分析

总辐射表夜间零点偏移试验在夜间晴天条件下,采用室外平行对比法对不同型号的总辐射表的零点进行测试。通过数据分析,分别比较了黑白型和全黑型总辐射表、国产与进口总辐射表夜间零点偏移的大小,并分析了形成零点偏移的原因。试验结果表明,在夜间晴天条件下国产总辐射表的零点偏移小于10 W·m~(-2)通过总辐射表感应面向下水平安装和加盖试验也验证了零点偏移确实是由"冷天空"所致。     

利用多角度POLDER偏振资料实现陆地上空大气气溶胶光学厚度和地表反照率的同时反演 I. 理论与模拟

陆地上空标量辐射对地表反射率和大气气溶胶散射都具有很强的敏感性,而偏振反射只对大气气溶胶敏感,对地表不敏感。根据这个原理并结合POLDER(POLarization and Directionality of Earth Reflectance)资料的特点,作者提出综合利用标量辐射和偏振反射信息来实现陆地上空大气气溶胶和地表反照率的同时反演。首先,利用多角度偏振辐射观测提取大气气溶胶光学参数,再利用标量辐射测量对偏振反演结果作进一步筛选和订正,同时获得地表反射率。数值模拟试验结果证明,仅利用偏振信息只能获取大气气溶胶信息,而且其结果误差较大,特别是对于散射作用较强的短波长通道如670 nm误差更大,但经过标量辐射订正后的结果得到明显改善,气溶胶光学厚度和地表反射率与真实值之间相关系数都达到0.99以上。为提高查找表的计算效率,提出并建立了反演方案所需要的半参数化数值表,利用内插方法寻求气溶胶光学厚度和地表反射率的数值解的反演方法。     

利用多角度POLDER偏振资料实现陆地上空大气气溶胶光学厚度和地表反照率的同时反演Ⅰ.理论与模拟

陆地上空标量辐射对地表反射率和大气气溶胶散射都具有很强的敏感性, 而偏振反射只对大气气溶胶敏感, 对地表不敏感.根据这个原理并结合POLDER (POLarization and Directionality of Earth Reflectance) 资料的特点, 作者提出综合利用标量辐射和偏振反射信息来实现陆地上空大气气溶胶和地表反照率的同时反演.首先, 利用多角度偏振辐射观测提取大气气溶胶光学参数, 再利用标量辐射测量对偏振反演结果作进一步筛选和订正, 同时获得地表反射率.数值模拟试验结果证明, 仅利用偏振信息只能获取大气气溶胶信息, 而且其结果误差较大, 特别是对于散射作用较强的短波长通道如670 nm误差更大, 但经过标量辐射订正后的结果得到明显改善, 气溶胶光学厚度和地表反射率与真实值之间相关系数都达到0.99以上.为提高查找表的计算效率, 提出并建立了反演方案所需要的半参数化数值表, 利用内插方法寻求气溶胶光学厚度和地表反射率的数值解的反演方法.     

FS-J1四分量净全辐射表在北极地区的性能评测

在全球变暖的背景下,全球的净全辐射监测越来越受到人们的重视,逐渐成为研究区域天气气候的重要手段。为了研究国产FS-J1型四分量净全辐射表在极地条件下的各项性能,于2017年4月10—23日在美国阿拉斯加巴罗地区(203.5°E,71.4°N)进行了为期2周的地面净全辐射量实时监测,并与极地地区应用较广的CNR4型四分量净全辐射表进行对比测试。结果表明:(1)在表面无结冰/霜条件下,国产仪器FS-J1型四分量净全辐射表在不同晴空和日夜条件下都表现出较好的精度和线性关系,各项参数与CNR4的相对误差和相关系数总体分别在5%以内和0.9以上。(2)受极地条件影响,FS-J1表面结冰/霜后,会对辐射变化的响应出现延迟,对总辐射表和地球辐射表分别能造成最大约25%和7%的相对误差。所以针对极地辐射站加设合适的通风加热装置、发展较为合理的误差订正方案仍是国产仪器以后需要改进的关键点。     

五九型探空仪温度湿度基值测定的分析

一、五九型探空仪温度湿度感应元件工作原理与误差概述 五九型探空仪温度感应元件是螺旋形双金属片。螺旋形双金属片由两种热膨胀系数不同的金属压制而成。主动片(里片)用膨胀系数较大的镍铬钢,被动片(外片)用膨胀系数较小的因瓦钢。当温度降低时,双金属片向内弯曲,反则,向外弯曲。同时,带动指针偏转。偏转后,指针尖接触电码滚筒的位置随之改变,发出不同的温度电码符号,表示周围的气温。     

GTS探空仪碳湿敏元件性能测试数据分析及相对湿度订正

碳湿敏元件受温度影响明显,造成相对湿度探空数据测量的误差。利用温湿控制设备对该元件进行静态试验,测试不同温度对元件感湿特性的影响。通过对试验数据分析计算得到元件的相对湿度温度项订正数据,以及相对湿度的温度项订正拟合公式,可以有效订正由温度引起的相对湿度探空数据误差。对实际相对湿度探空数据资料订正效果的对比分析表明,经过温度项订正后的相对湿度探空数据,不但其准确度得到了提高,而且清楚地体现出在订正之前所不能体现的高空大气相对湿度在低湿段的变化细节。     

计算非均一大气条件下太阳辐射通量的一个简单而又精确的模式

发展了一个计算非均一大气条件下太阳辐射通量的一个简单而又精确的模式，其中包括关于大气球反射率与透过率的一个参数化表达式，并引入加权一次散射反照率和加权不对称因子，用于拟合非均一大气条件下计算辐射通量的四个经验订正因子。对清洁和浑浊的两类大气，都具有120060组的辐射通量模拟试验，以检验本模式的精度。这些模拟试验覆盖0－50的云光学厚度、0－0．8地表反射率、Junge和对数正态的气溶胶谱分布、－0．05气溶胶折射率虚部。在均一大气条件下，由本模式计算的120060组向上通量的标准差对清洁和浑浊两类大气分别为1．08％和1．04％；而向下通量的标准差分别为4.12%和3．31％。在非均一大气条件下，由本模式计算的向上通量的标准差对清洁和浑浊两类大气分别为3．01％和3．48％；而向下通量的标准差分别为4．54％和4．89％，其精度远优于均一假设下的计算结果。     

快速为直接辐射表对光点

2001年6月直接辐射表换型后,许多观测员反映对光点比较困难.我们在实践中总结出巧对光点的方法:首先,对准时间,即让直接辐射表下边的时间指针指向直表钟机上的观测时间;第二步,对准方位,即用一小片较薄的白纸,在白纸上挖一小洞,让小洞与直接辐射表光环上的黑点重叠,然后调整直表方位.这样很容易看清光线是否透过小孔落在黑点上(即对准光点).     

强制通风温度传感器的计算流体动力学分析

本文利用计算流体动力学(Computational Fluid Dynamics, CFD)方法对基于076B型强制通风防辐射罩的温度传感器进行流固耦合传热分析,计算不同太阳辐射强度、下垫面反射率、强制通风速度、气象站海拔高度和下垫面长波辐射强度等影响因子条件下温度传感器的辐射误差。为实现影响因子连续变化时能提供准确修正数据的目标,采用神经网络算法仿真值计算结果进行拟合,获得辐射误差订正方程。结果表明,辐射误差订正方程的修正误差在0.005℃以内。订正后的气温观测数据有望用于气候变化研究和高精度天气预报。     

南极中山站太阳紫外辐射测值比较

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。     

Radiometric Cross-Calibration for Multiple Sensors with the Moon as an Intermediate Reference

The instrument cross-calibration is an effective way to assess the quality of satellite data. In this study, a new method is proposed to cross-calibrate the sensors among satellite instruments by using a RObotic Lunar Observatory(ROLO) model and Apollo sample reflectance in reflective solar bands(RSBs). The ROLO model acts as a transfer radiometer to bridge between the instruments. The reflective spectrum of the Apollo sample is used to compensate for the difference in the instrument's relative spectral responses(RSRs). In addition, the double ratio between the observed lunar irradiance and the simulated lunar irradiance is used to reduce the difference in instrument lunar viewing and illumining geometry. This approach is applied to the Moderate Resolution Imaging Spectroradiometer(MODIS), the Sea-Viewing Wide Field-of-View Sensor(Sea Wi FS), and the Advanced Land Imager(ALI) on board three satellites, respectively. The mean difference between MODIS and Sea Wi FS is less than 3.14%, and the difference between MODIS and ALI is less than 4.75%. These results indicate that the proposed cross-calibration method not only compensates for the RSR mismatches but also reduces the differences in lunar observation geometry. Thus,radiance calibration of any satellite instrument can be validated with a reference instrument bridged by the moon.     

5种光合有效辐射表性能测试

为认识和提高光合有效辐射 (波长为400~700 nm) 的测量精度,对国内外5种常用的光合有效辐射表的灵敏度、余弦响应、非线性、温度依赖性、光谱响应等性能进行了测试和分析。结果表明: 5种光合有效辐射表 (简称光合表) 的非线性误差均在1%以内; 3种光合表 (PAR LITE,LI-190和FS-PR) 的余弦误差均小于10%,温度系数均小于0.3%/℃,2种光合表 (TRT-5和HSC-FPH-1) 的余弦误差明显偏大,温度系数小于0.5%/℃。2种光合表 (PAR LITE和LI-190) 的光谱响应曲线接近于理想光谱,而其余3种光合表与理想光谱曲线偏离较大。在自然光下的一致性比对测量结果显示,5种光合表测量的辐射量与标准值的误差均在5%以内,但综合评价后认为,3种光合表 (PAR LITE,LI-190和FS-PR) 的性能明显优于其他2种光合表 (TRT-5和HSC-FPH-1)。该结果可为气象观测业务选型提供参考。     

Out-of-Range Stray Light Characterization of Single-Monochromator Brewer Spectrophotometers

Stray light in single-monochromator Brewer instruments increases the uncertainty of solar ultraviolet spectral irradiance measurements and ozone retrievals. To study how spectral irradiance within and outside the measurement ranges of the instruments affects stray light, two Brewer MKII instruments were characterized for the level of in- and out-of-range stray light at multiple laser wavelengths. In addition, several solar-blind filters utilized in single-monochromator Brewers to limit out-of-range stray light were characterized for spectral and spatial transmittances. Finally, the measurement results were used to simulate the effect of stray light and stray light correction on spectral irradiance and ozone measurements at different wavelength regions. The effect of stray light from wavelengths above 340?nm was found to be negligible compared with other sources of uncertainty. On the other hand, contributions from wavelengths between 325 and 340?nm can form a significant portion of the overall stray light of the instrument, with 325?nm being the upper limit of the nominal measurement range of the instrument.     

Effects of cloudiness on global and diffuse UV irradiance in a high-mountain area

Summary At the high-mountain station Jungfraujoch (3576 m a.s.l., Switzerland), measurements of the radiation fluxes were made during 16 periods of six to eight weeks by means of a Robertson—Berger sunburn meter (UVB data), an Eppley UVA radiometer and an Eppley pyranometer. Cloudiness, opacity and altitude of clouds were recorded at 30-minute intervals. A second set of instruments was employed for separate measurement of the diffuse radiation fluxes using shadow bands. The global and diffuse UVA- and UVB radiation fluxes change less with cloudiness than the corresponding total radiation fluxes. When the sun is covered by clouds, the global UVA- and UVB radiation fluxes are also affected less than the global total radiation flux. The roughly equal influence of cloudiness on the UVA- and UVB radiation fluxes suggests that the reduction is influenced more by scattering than by ozone. Also, the share of diffuse irradiance in global irradiance is considerably higher for UVA- and UVB irradiance than for total irradiance. At 50° solar elevation and 0/10 cloudiness, the share is 39% for UVB irradiance, 34% for UVA irradiance and 11% for total irradiance. The increased aerosol turbidity after the eruptions of El Chichon and Pinatubo has caused a significant increase in diffuse total irradiance but has not produced any significant changes in diffuse UVA- and UVB irradiances.With 7 Figures     

Ultraviolet sky radiance distributions of translucent overcast skies

Summary The diffuse sky radiation component in the ultraviolet wavelengths is often at least 50% of the global irradiance under clear skies, and is the dominant component of ultraviolet global radiation under translucent overcast skies. The distribution of sky radiance was measured in a rural area and modeled for wavelength bands of ultraviolet-B (UVB, 280–320 nm) and ultraviolet-A (UVA, 320–400 nm). Sky radiance measurements were made during the summer of 1993 over a wide range of solar zenith angles using radiance sensors mounted on a hand-operated hemispherical rotation mount. UVB irradiance measurements were also made during each scan. Since the ratio of measured irradiance under overcast skies and that predicted for clear skies was not correlated with cloud base height, opaque cloud fraction, or solar zenith angle, it was concluded that the scattering from the clouds dominated the global irradiance, and this scattering was relatively unaffected by the scattering off opaque clouds in the translucent atmosphere.Analysis of the translucent overcast sky UVA and UVB radiance measurements using a semi-empirical distribution model showed that the spectral influences on multiple scattering, single scattering, and horizon brightening components of the distributions agreed with basic atmospheric radiation theory. The best model used solar zenith, the sky zenith, and the scattering angle with resultant coefficient of determination values of 0.62 and 0.25 for the UVA and UVB respectively. The developed equations can be applied directly to the diffuse sky irradiance on the horizontal to provide radiance distributions for the sky.With 6 Figures     

气象卫星可见光红外光学成像仪发展沿革

该文回顾了环境气象卫星可见光红外光学成像遥感仪器50多年的发展历程,从不同时期在轨运行的近百台 (套) 仪器中选择了12种作为代表,结合仪器功能性能技术指标和应用需求梳理分析了其历史发展脉络和主流业务发展趋势,并初步探讨了创新发展方向。50多年的发展可以分为3个阶段:早期探索20年, 美国第1代探索性仪器,开创了气象卫星对地观测的先河;初步应用20年, 基本形成初步应用格局,欧洲、中国等开始发展自己的环境气象卫星光学成像遥感仪器;稳定应用和进步发展10多年。新一代极轨卫星可见光红外光学成像遥感仪器,其典型特征是光谱波段20个以上,谱段带宽窄,光谱范围全面覆盖0.4~15 μm,辐射测量精度高,空间分辨率为200~1000 m,其改进型仪器代表了未来极轨气象卫星主流业务发展趋势。静止气象卫星可见光红外光学成像遥感仪器未来主流业务发展方向的典型特点是光谱波段15个以上,谱段带宽较窄,光谱范围全面覆盖0.4 ~15 μm,辐射测量精度高,空间分辨率为500~2000 m,圆盘图成像速度可达到分钟级,区域扫描速度更快。     

Measurements of chemically and biologically effective radiation reaching the ground

Solar ultraviolet radiation at the surface has been measured at Potsdam on cloudless days by spectrometer OL 752/10. The measurements are compared with broad-band filter measurements and with model calculations using a modified version of Green's model, which is independent of the measurements. Input data to the model such as atmospheric ozone and aerosol optical thicknesses were measured by a Dobson and Brewer spectrophotometer as well as a Linke Feussner pyrheliometer, respectively. Differences between the model and the measurements are discussed in terms of uncertainties in the calibration and errors of instruments as well as uncertainties in the model calculations including the errors of input data. It is demonstrated that different chemically and biologically effective radiances can be determined from only one set of measured spectral irradiance components, i.e. global radiation and diffuse downward and upward directed radiation. Examples of diurnal variations of the photochemical production of ozone and hydroxyl radicals as determined from spectral irradiance measurements and measured concentrations of relevant trace gases are given.It is shown from the measured irradiance that relations between different effects of radiation to the biosphere depend on solar zenith angle, and to a certain extent also on atmospheric ozone. This has to be taken into account when adverse effects of changing UV radiation are evaluated. Radiation Amplification Factors derived from measurements correspond to those determined from model calculations.     

湿度表(计)检定装置不确定度分析

湿度检定装置的不确定度,直接影响到湿度传感器和各种湿度测量仪器的检测结果。该文针对我国省级气象计量单位,现用的湿度表（计）检定装置,从检定装置的组成、主要误差来源及分类人手,借鉴国内外通用的不确定度分析方法,介绍整个湿度检定装置的不确定度测试与评估。     

Aerosol optical properties during Asian dust storm episodes in South Korea

Summary ¶Aerosol optical depth (_a) is the most comprehensive variable to characterize aerosol, assess atmospheric pollution and make atmospheric corrections to satellite remotely sensed data from ground-based instruments. The aerosol optical properties in Korea peninsula observed at both Kwangju and Anmoyondo during the Asian dust period (March–May) have been presented in this study. Aerosol optical depths at all wavelengths showed a sharp increase during major dust outbreak in spring when compared with the average for the season. For example at Kwangju, aerosol optical depths increase from the spring average value of 0.43±0.02 at 501nm to values >0.70 during major dust event days in 1999 and 2001. Daily mean Ångström exponents () computed at both sites show dramatic changes from high values to low values on dust day periods with a sharp increase in the single scattering albedo. The study also revealed that the observed direct normal solar irradiance and diffuse horizontal irradiance during days with increased dust pollution levels is capable of reducing direct solar radiation by as much as 28% and a corresponding increase of 14% in diffuse solar irradiance during cloudless and windless days.