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A large-area blackbody for in-flight calibration of an infrared interferometer deployed on board a long-duration balloon for stratospheric research

机译:大面积黑体,用于在飞行中校准红外干涉仪,该红外干涉仪部署在长气球上进行平流层研究

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The deployment of the imaging Fourier Transform Spectrometer GLORIA (Gimballed Limb Observer for Radiance Imaging of the Atmosphere) on board a long-duration balloon for stratospheric research requires a blackbody for in-flight calibration in order to provide traceability to the International Temperature Scale (ITS-90) to ensure comparability with the results of other experiments and over time. GLORIA, which has been deployed onboard various research aircraft such as the Russian M55 Geophysica or the German HALO in the past, shall also be used for detailed atmospheric measurements in the stratosphere up to 40 km altitude. The instrument uses a two-dimensional detector array and an imaging optics with a large aperture diameter of 36?mm and an opening angle of 4.07 sup°/sup × 4.07 sup°/sup for infrared limb observations. To overfill the field of view (FOV) of the instrument, a large-area blackbody radiation sources (125 mm × 125 mm ) is required for in-flight calibration. In order to meet the requirements regarding the scientific goals of the GLORIA missions, the radiance temperature of the blackbody calibration source has to be determined to better than 100 mK and the spatial temperature uniformity shall be better than 150 mK . As electrical resources on board a stratospheric balloon are very limited, the latent heat of the phase change of a eutectic material is utilized for temperature stabilization of the calibration source, such that the blackbody has a constant temperature of about ? 32 sup°/supC corresponding to a typical temperature observed in the stratosphere. The Institute for Atmospheric and Environmental Research at the University of Wuppertal designed and manufactured a prototype of the large-area blackbody for in-flight calibration of an infrared interferometer deployed on board a long-duration balloon for stratospheric research. This newly developed calibration source was tested under lab conditions as well as in a climatic and environmental test chamber in order to verify its performance especially under flight conditions. At the PTB (Physikalisch-Technische Bundesanstalt), the German national metrology institute, the spatial radiance distribution of the blackbody was determined and traceability to the International Temperature Scale (ITS-90) has been assured. In this paper the design and performance of the balloon-borne blackbody (BBB) is presented.
机译:成像傅里叶变换光谱仪GLORIA(用于大气辐射成像的球形四肢观察者)部署在用于平流层研究的长时程气球上,需要黑体进行飞行中校准,以提供对国际温度标度(ITS)的可追溯性-90),以确保与其他实验的结果具有可比性。 GLORIA过去曾被部署在各种研究飞机上,例如俄罗斯的M55地球物理公司或德国的HALO,也将用于高达40 km高度的平流层中详细的大气测量。该仪器使用二维检测器阵列和成像光学器件,孔径为36?mm,开口角度为4.07 °×4.07 ° 。为了使仪器的视场(FOV)充满,在飞行中校准需要大面积的黑体辐射源(125 mm×125 mm)。为了满足有关GLORIA任务的科学目标的要求,黑体校准源的辐射温度必须确定为高于100 mK,空间温度均匀性应高于150 mK。由于平流层气球上的电力资源非常有限,因此将低共熔材料相变的潜热用于校准源的温度稳定化,以使黑体的恒定温度约为? 32 ° C对应于平流层中观察到的典型温度。伍珀塔尔大学大气与环境研究所设计并制造了大面积黑体的原型,该原型用于在飞行中校准部署在用于平流层研究的长时气球上的红外干涉仪。为了验证其性能,特别是在飞行条件下,已在实验室条件以及气候和环境测试室内对这种新开发的校准源进行了测试。在德国国家计量研究所的PTB(Physikalisch-Technische Bundesanstalt),确定了黑体的空间辐射分布,并确保了可追溯至国际温度标度(ITS-90)。本文介绍了球囊黑体(BBB)的设计和性能。

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