共查询到19条相似文献,搜索用时 171 毫秒
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JJG 211-2005亮度计检定规程已颁布实施,它同时囊括了亮度计和彩色亮度计的检定,增加了光源色度参数的校准.在实施实践中,校准彩色亮度计所用的标准反射色板采用了色差计校准用的一套标准反射色板,校准时的标准值取标准反射色板溯源证书中的A/2,0/45的数据.从彩色亮度计中光源色度参数的实验数据,以及对其测量结果的不确定度分析,均证明新规程校准方法正确,而共用标准反射色板亦可行,校准效果良好. 相似文献
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光电转速表测量范围大,准确度高,在企事业单位应用广泛,但自行校准比较困难。本文简要介绍了光电转速表中转速传感器及二次仪表的工作原理,对采用脉冲光源法校准光电转速表的测量方法进行了探讨,阐述了使用频闪式转速表作为脉冲光源校准光电转速表的校准方法和有关注意事项。 相似文献
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介绍一种浮空器气囊体积测量装置的现场校准方法,通过设定现场校准区域,构建地面控制点的局部三维坐标;在被测对象侧边的6个地面控制点设立测站,用激光全站仪和棱镜组件按照极坐标法观察得到被测对象侧边精密标定杆上所有准校点的局部三维坐标,建立校准参考坐标系,构建完整的现场校准场。测量装置对在校准参考坐标系中的精密标定杆上校准点进行拍摄获得图片,解算得到测量装置的每个相机的外方位元素,得到其位置和姿态,完成校准工作。本文提出的现场校准方法解决了测量装置在任意场景下浮空器囊体体积测量的应用问题和测量装置使用中需要搬动情况下的校准问题。 相似文献
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传统振弦式应变计校准装置一般采用人力或小功率电机驱动作为驱动力,难以满足需施加大测力的振弦式应变计校准要求。基于此,设计并研制了一种基于液压驱动的振弦式应变计校准装置,以解决大测力振弦式应变计难校准的问题。校准装置可以在50~200 mm范围内调整,设计了通用夹具来实现不同尺寸、不同型号和不同形状振弦式应变计的装夹紧固。该装置结构紧凑,操作便利省力,经验证液压驱动在极大减轻校准所需施加力的同时,校准结果与传统应变计测量数据相一致,验证实验的测量不确定度U=0.6%(k=2),小于0.7%,满足校准规范要求。 相似文献
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For instruments that carry onboard solar diffusers to orbit, such as the Sea-Viewing Wide Field-of-View Sensor (SeaWiFS), it is possible to convert the instrument's reflectance measurements to radiance measurements by knowledge of the solar irradiance. This process, which generally requires the application of a solar irradiance model, is described. The application of the irradiance model is separate from the measurements by the instrument and from the instrument's reflectance calibration. In addition, SeaWiFS was calibrated twice before launch for radiance response by use of radiance sources with calibrations traceable to the National Institute of Standards and Technology. With the inclusion of the at-launch diffuser-based radiance calibration, SeaWiFS has three possible radiance calibrations forthe start of on-orbit operations. The combination of these three into a single calibration requires changes of 4% or less for the current at-launch radiance calibration of the instrument. Finally, this process requires changes of 4% or less for the reflectance calibration coefficients to provide consistency among the radiance calibration, the reflectance calibration, and the solar irradiance. 相似文献
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Edward A. Early Ambler Thompson 《Journal of research of the National Institute of Standards and Technology》1996,101(2):141-153
Spectral irradiance calibrations often require that irradiance standard lamps be oriented differently than the normal calibration orientation used at the National Institute of Standards and Technology and at other standards laboratories. For example, in solar measurements the instruments are generally upward viewing, requiring horizontal working standards for minimization of irradiance calibration uncertainties. To develop a working standard for use in a solar ultraviolet intercomparison, NIST determined the irradiance of quartz-halogen lamps operating in the horizontal position, rather than in the customary vertical position. An experimental technique was developed which relied upon equivalent lamps with independent mounts for each orientation and a spectroradiometer with an integrating sphere whose entrance port could be rotated 90° to view either lamp position. The results presented here are limited to 1000 W quartz-halogen type lamps at ultraviolet wavelengths from 280 nm to 400 nm. Sources of uncertainty arose from the lamps, the spectroradiometer, and the lamp alignment, and increased the uncertainty in the irradiance of horizontal lamps by less than a factor of two from that of vertical NIST standard lamps. The irradiance of horizontal lamps was less than that of vertical lamps by approximately 6 % at long wavelengths (400 nm) to as much as 12 % at the shortest wavelengths (280 nm). Using the Wien radiation law, this corresponds to color temperature differences of 15.7 K and 21.3 K for lamps with clear and frosted envelopes, respectively. 相似文献
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标准太阳电池的短路电流可用来确定太阳模拟器的总辐照度强度。选取单晶硅、多晶硅、非晶硅薄膜和染料敏化4种常见类型的太阳电池,分别进行光谱响应度测量。对光谱匹配分别为A、B、C级的太阳模拟器进行光谱辐照度分布测量。利用光谱失配计算公式,并结合标准AM1.5G太阳光谱辐照度分布数据,理论计算出由于光源间光谱不匹配以及电池间光谱响应度不匹配所产生的光谱失配因子,并对标定太阳电池产生的影响进行了分析。 相似文献
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A radiometrically stable, commercially available spectroradiometer was used in conjunction with a simple, custom-designed telescope to make spectrally continuous measurements of solar spectral transmittance and directly transmitted solar spectral irradiance. The wavelength range of the instrument is 350-2500 nm and the resolution is 3-11.7 nm. Laboratory radiometric calibrations show the instrument to be stable to better than 1.0% over a nine-month period. The instrument and telescope are highly portable, can be set up in a matter of minutes, and can be operated by one person. A method of absolute radiometric calibration that can be tied to published top-of-the-atmosphere (TOA) solar spectra in valid Langley channels as well as regions of strong molecular absorption is also presented. High-altitude Langley plot calibration experiments indicate that this technique is limited ultimately by the current uncertainties in the TOA solar spectra, approximately 2-3%. Example comparisons of measured and modtran-modeled direct solar irradiance show that the model can be parameterized to agree with measurements over the large majority of the wavelength range to the 3% level for the two example cases shown. Side-by-side comparisons with a filter-based solar radiometer are in excellent agreement, with a mean absolute difference of tau = 0.0036 for eight overlapping wavelengths over three experiment days. 相似文献
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Edward Early Ambler Thompson Carol Johnson John DeLuisi Patrick Disterhoft David Wardle Edmund Wu Wanfeng Mou Yongchen Sun Timothy Lucas Tanya Mestechkina Lee Harrison Jerry Berndt Douglas S. Hayes 《Journal of research of the National Institute of Standards and Technology》1998,103(1):15-62
Concern over stratospheric ozone depletion has prompted several government agencies in North America to establish networks of spectroradiometers for monitoring solar ultraviolet irradiance at the surface of the Earth. To assess the ability of spectroradiometers to accurately measure solar ultraviolet irradiance, and to compare the results between instruments of different monitoring networks, the second North American Intercomparison of Ultraviolet Monitoring Spectroradiometers was held June 12 to 23, 1995 at Table Mountain outside Boulder, Colorado, USA. This Intercomparison was coordinated by the National Institute of Standards and Technology (NIST) and the National Oceanic and Atmospheric Administration (NOAA). Participating agencies were the Environmental Protection Agency; the National Science Foundation; the Smithsonian Environmental Research Center; the Department of Agriculture; and the Atmospheric Environment Service, Canada. Instruments were characterized for wavelength uncertainty, bandwidth, stray-light rejection, and spectral irradiance responsivity, the latter with a NIST standard lamp operating in a specially designed field calibration unit. The spectral irradiance responsivity, determined once indoors and twice outdoors, demonstrated that while the responsivities changed upon moving the instruments, they were relatively stable when the instruments remained outdoors. Synchronized spectral scans of the solar irradiance were performed over several days. Using the spectral irradiance responsivities determined with the NIST standard lamp and three different convolution functions to account for the different bandwidths of the instruments, the measured solar irradiances generally agreed to within 3 %. 相似文献
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Edward Early Ambler Thompson Carol Johnson John DeLuisi Patrick Disterhoft David Wardle Edmund Wu Wanfeng Mou James Ehramjian John Tusson Tanya Mestechkina Mark Beaubian James Gibson Douglass Hayes 《Journal of research of the National Institute of Standards and Technology》1998,103(5):449-482
Concern over stratospheric ozone depletion has prompted several government agencies in North America to establish networks of spectroradiometers for monitoring solar ultraviolet irradiance at the surface of the Earth. To assess the ability of spectroradiometers to accurately measure solar ultraviolet irradiance, and to compare the results between instruments of different monitoring networks, the third North American Interagency Intercomparison of Ultraviolet Monitoring Spectroradiometers was held June 17–25, 1996 at Table Mountain outside Boulder, Colorado, USA. This Intercomparison was coordinated by the National Institute of Standards and Technology (NIST) and the National Oceanic and Atmospheric Administration (NOAA). Participating agencies were the Environmental Protection Agency; the National Science Foundation; the Smithsonian Environmental Research Center; the Department of Agriculture; and the Atmospheric Environment Service, Canada. The spectral irradiances of participants’ calibrated standard lamps were measured at NIST prior to the Intercomparison. The spectral irradiance scales used by the participants agreed with the NIST scale within the combined uncertainties, and for all lamps the spectral irradiance in the horizontal position was lower than that in the vertical position. Instruments were characterized for wavelength uncertainty, bandwidth, stray-light rejection, and spectral irradiance responsivity, the latter with NIST standard lamps operating in specially designed field calibration units. The spectral irradiance responsivity demonstrated instabilities for some instruments. Synchronized spectral scans of the solar irradiance were performed over several days. Using the spectral irradiance responsivities determined with the NIST standard lamps, the measured solar irradiances had some unexplained systematic differences between instruments. 相似文献
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A technique for calibrating spectral radiometers measuring global (2π sr) irradiance using solar irradiance at the top of the atmosphere as the absolute irradiance reference is reported. In addition to providing a calibration at all measured wavelengths, the technique provides a direct measure of the angular response of the radiometer. For instruments that can be used to measure the ultraviolet-B region, the calibration also provides an estimate of the ozone column amount. 相似文献