精度:立方体卫星辐射计星座的自适应校准

John W. Bradburn, M. Aksoy, Henry R. Ashley
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引用次数: 3

摘要

传感技术的最新进展使配备辐射计的立方体卫星能够用于科学任务。虽然立方体卫星星座为遥感科学任务提供了好处,但由于对环境条件相当敏感,它们也带来了校准方面的独特挑战。为了解决这个问题,正在开发一个星座级校准框架,称为“立方体卫星辐射计星座自适应校准(精度)”。该框架处于早期阶段,目前通过使用合成数据的初始端到端原型覆盖理论基础。该框架将使用发射前和在轨收集的仪器级遥测数据,将星座成员分离为处于相似状态的时间适应辐射计组(或集群)。在集群内,所有辐射计将其绝对校准测量值共享到一个公共校准数据池。这些校准池包含不同校准目标在不同时间的测量结果,方便频繁的多点绝对校准。这反过来又有助于减少和量化校准误差和不确定性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
ACCURACy: Adaptive Calibration of CUbesat RAdiometer Constellations
Recent advances in sensing technology have enabled the deployment of CubeSats equipped with radiometers for scientific missions. While constellations of CubeSats provide benefits to remote sensing science missions, they also bring with them unique challenges in calibration due to considerable sensitivity to ambient conditions. To address this problem, a constellation-level calibration framework is being developed, called “Adaptive Calibration of CUbesat RAdiometer Constellations (ACCURACy)”. This framework is in early stages, currently covering the theoretical basis through an initial end-to-end prototype utilizing synthetic data. This framework will use instrument-level telemetry data collected pre-launch and in-orbit to separate constellation members into time-adaptive groups (or clusters) of radiometers in similar states. Within clusters, all radiometers share their absolute calibration measurements to a common calibration data pool. These calibration pools, containing measurements of different calibration targets at different times, facilitate frequent multi-point absolute calibration. This, in turn, serves to reduce and quantify calibration errors and uncertainties.
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