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In orbit validation of the Sentinel 5 Precursor TROPOMI earth observation instrument thermal control system

机译:在Sentinel 5前体验证的轨道验证中,Precoroor Tropomi Ared Abservation仪器热控制系统

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The Tropospheric Monitoring Instrument (TROPOMI) on ESAs Sentinel 5 Precursor spacecraft was launched on October 13th 2017. Sentinel-5 Precursor is an ESA mission on behalf of the European Commission. The TROPOMI instrument has been developed under instrument prime responsibility of AIRBUS Defence and Space Netherlands BV and is jointly funded by ESA and the Kingdom of the Netherlands with NL Programme management by the Netherlands Space Office (NSO). The mission of this instrument is to perform observations on air quality and on sources and sinks of air quality and climate related gases and aerosols. TROPOMI is a passive Solar backscatter imaging spectrometer sensitive in several spectral bands from ultraviolet (UV) to Short Wave Infrared (SWIR), allowing deep penetration into the atmosphere, observing scattered radiation close to the Earth's surface. The instrument's spatial resolution of 7 x 7 km2 results in a high fraction of cloud-free observations. The wide swath range allows daily Earth coverage. The four 2D detectors in the instrument (SWIR, NIR, UVIS, UV) are cooled down to temperature levels varying from 140 K to 210 K to reduce the dark current output. This paper focuses on the in-orbit thermal observations, the correlation with the thermal predictions and the applied fine-tuning of the parameters in the active thermal control systems. Based on the correlated thermal model and in orbit observations, the extreme lifetime excursions have been re-assessed. The outcome of the in orbit validation has been used to define the final settings for the thermal control system in order to ensure full performance during the entire life time.
机译:欧空局哨兵5前体飞船对流层监测仪(TROPOMI)于10月13日2017年推出的Sentinel-5前体是代表欧盟委员会的欧空局的使命。 Tropomi仪器已经在仪器防御和空间荷兰BV的仪器责任下开发,并由荷兰航天局(NSO)的NL计划管理是共同的ESA和荷兰王国资助的。该仪器的使命是对空气质量和气体质量和气候相关气体和气溶胶汇进行的观察。 Tropomi是一种被动太阳能反向散射成像谱仪,其在来自紫外线(UV)到短波红外(SWIR)的多个光谱带中,允许深入渗透到大气中,观察靠近地球表面的散射辐射。仪器的空间分辨率为7 x 7平方公里,导致云观测的高分。宽的条子距离允许每日地球覆盖范围。仪器(SWIR,NIR,UVI,UV)中的四个2D检测器被冷却至从140k到210k变化的温度水平,以减少暗电流输出。本文重点介绍了轨道热观察,与热预测的相关性和有源热控制系统中的参数的应用微调。基于相关的热模型和轨道观测,重新评估了极端的寿命偏移。在轨道验证的结果已用于定义热控制系统的最终设置,以确保在整个寿命期间的完整性能。

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