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The in-flight blackbody calibration system for the GLORIA interferometer on board an airborne research platform

机译:机载研究平台上用于GLORIA干涉仪的机上黑体校准系统

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The bG/bimballed bL/bimb bO/bbserver for bR/badiance bI/bmaging of the bA/btmosphere (GLORIA) is a prototype of an imaging Fourier Transform Spectrometer (FTS) for PREMIER, a former candidate mission for ESA's Earth Explorer 7. GLORIA is deployed on board various research aircraft such as the Russian M55 Geophysica or the German HALO. The instrument provides detailed infrared images of the Upper Troposphere/Lower Stratosphere (UTLS) region, which plays a crucial role in the climate system. GLORIA uses a two-dimensional detector array for infrared limb observations in emission and therefore needs large-area blackbody radiation sources (126 mm ?? 126 mm) for calibration. brbr In order to meet the highly demanding uncertainty requirements for the scientific objectives of the GLORIA missions and due to the sophisticated tomographic evaluation scheme, the spatial distribution of the radiance temperature of the blackbody calibration sources has to be determined with an uncertainty of about 0.1 K. Since GLORIA is exposed to the hostile environment of the UTLS with mutable low temperature and pressure, an in-flight calibration system has to be carefully designed to cope with those adverse circumstances. brbr The GLORIA in-flight calibration system consists of two identical weight-optimised high-precision blackbody radiation sources, which are independently stabilised at two different temperatures. The two point calibration is in the range of the observed atmospheric infrared radiance emissions with 10 K below and 30 K above ambient temperature, respectively. Thermo-Electric Coolers are used to control the temperature of the blackbody radiation sources offering the advantage of avoiding cryogens and mechanical coolers. The design and performance of the GLORIA in-flight calibration system is presented. The blackbody calibration sources have been comprehensively characterised for their spatially (full aperture) and spectrally (7 to 13 ??m) resolved radiation properties in terms of radiance temperatures traceable to the International Temperature Scale (ITS-90) at the Physikalisch-Technische Bundesanstalt (PTB), the national metrology institute of Germany.
机译:G 标记的 L imb O 观察者,用于 R 辅助 I b> A tmosphere(GLORIA)是PREMIER成像傅立叶变换光谱仪(FTS)的原型,该成像仪是ESA Earth Explorer 7的前任任务。GLORIA部署在各种研究飞机上,例如俄罗斯M55地球物理学或德国的HALO。该仪器提供了对流层上层/平流层下层(UTLS)区域的详细红外图像,这在气候系统中起着至关重要的作用。 GLORIA使用二维检测器阵列来观察发射中的红外肢体,因此需要大面积的黑体辐射源(126 mm≤126 mm)进行校准。 为了满足GLORIA任务的科学目标的高度不确定性要求,并且由于复杂的层析成像评估方案,黑体校准源的辐射温度的空间分布必须使用不确定性约为0.1K。由于GLORIA暴露于UTLS恶劣的低温和高压环境中,因此必须精心设计机内校准系统以应对这些不利情况。 GLORIA机内校准系统由两个相同的重量优化的高精度黑体辐射源组成,它们分别在两个不同的温度下稳定。两点校准分别在观察到的大气红外辐射发射范围内,分别低于环境温度10 K和高于环境温度30K。热电冷却器用于控制黑体辐射源的温度,具有避免制冷剂和机械冷却器的优势。介绍了GLORIA机内校准系统的设计和性能。黑体校准源的空间(全孔径)和光谱(7至13?m)分辨的辐射特性已经得到了全面表征,其辐射温度可追溯至Physikalisch-Technische Bundesanstalt的国际温度标度(ITS-90)。 (PTB),德国国家计量学会。

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