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Étalonnage au sol de l’instrument SIMBIO-SYS à bord de la mission ESA/BEPICOLOMBO

机译:ESA / BEPICOLOMBO任务上的SIMBIO-SYS仪器的地面校准

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摘要

BepiColombo is one of the cornerstones of the scientific program of ESA. It will study the planet Mercury with two spacecrafts in orbit around the planet. One of the two spacecrafts, the Mercury Planetary Orbiter (MPO), will be dedicated to the study of the surface and interior of the planet. The mission is scheduled for launch in 2016 and arrival at Mercury in January 2024. IAS is responsible for the calibration of the imaging system SIMBIO-SYS (Spectrometers and Imagers for MPO BepiColombo Integrated Observatory-SYStem) which consists of a high-resolution camera (HRIC), a stereoscopic camera (STC) and a visible and near-infrared hyperspectral imager (VIHI). These instruments should deeply change our understanding of the composition and geomorphology of Mercury surface. My research subject allowed me to participate in all the activities concerning the definition, implementation and validation of the calibration facilities at the IAS. These facilities are divided into different sub-systems: a thermal vacuum chamber containing the instrument during all the calibration campaign that shall simulate the environmental conditions (temperature and pressure), an optical bench with optical components and radiometrically calibrated sources reproducing the observational conditions as it will be seen by the instrument once placed in Mercury’s orbit, mechanical interfaces allowing the positioning and guidance of the instrument when placed inside the vacuum chamber with the required precision and accuracy, thermal interfaces facilitating the thermal excursion of the detectors, software interfaces so as to automatize and control the entire system. I developed a radiometric model of the calibration system and instrument to refine the calibration sources. In parallel, I performed several measurements of some subsystems so as to validate the optical assembly and to improve its control. Finally as a result of a close collaboration with the three Italian scientific teams of the instrument, I elaborate the fully package of the calibration sequences and the detailed instrument configuration that will be used during the calibration campaign.
机译:BepiColombo是ESA科学计划的基石之一。它将用两颗绕地球轨道飞行的航天器研究水星。水星行星轨道器(MPO)是两个航天器之一,将致力于研究行星的表面和内部。该任务计划于2016年发射,并于2024年1月到达水星。IAS负责对成像系统SIMBIO-SYS(用于MPO BepiColombo综合天文台-SYStem的光谱仪和成像仪)进行校准,该系统由高分辨率相机( HRIC),立体相机(STC)和可见光和近红外高光谱成像仪(VIHI)。这些仪器应该深刻改变我们对水银表面组成和地貌的理解。我的研究课题使我能够参与有关IAS校准设施的定义,实施和验证的所有活动。这些设施分为不同的子系统:在所有校准过程中均包含仪器的热真空室,该仪器应模拟环境条件(温度和压力),带有光学组件的光具座以及经过辐射校准的源,它们在再现时会产生观测条件。一旦放置在水星的轨道上,仪器将可以看到它,机械接口允许以所需的精度和准确性将仪器放置在真空室内时进行定位和引导,热接口有助于探测器的热漂移,软件接口可以自动化和控制整个系统。我开发了校准系统和仪器的辐射模型,以完善校准源。同时,我对一些子系统进行了几次测量,以验证光学组件并改善其控制能力。最后,由于与仪器的三个意大利科学团队紧密合作,我详细阐述了校准序列的完整软件包以及将在校准活动中使用的详细仪器配置。

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    Rodriguez-Ferreira Julian;

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  • 年度 2015
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