用于地球辐射收支的扫描辐射计的第一性原理动态电热数值模型

A. Ashraf, K. Priestley, J. Mahan
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引用次数: 0

摘要

地球观测仪器用于监测来自近地轨道的太阳辐射和长波辐射,在过去三十年中一直是研究地球辐射收支的重要组成部分。诸如此类的仪器要经过几个稳健的设计阶段,然后进行有力的地面校准活动,以在光谱、空间、时间和辐射学上设置其基线特征。从制造和校准这些仪器中获得的知识有助于技术进步,因为开发更精确仪器的需求增加了。为了了解仪器发射前的性能,NASA兰利研究中心与弗吉尼亚理工大学热辐射小组合作开发了扫描辐射计的第一性原理、动态电热数值模型,该模型可用于增强对轨道上类似地球辐射预算的仪器的解释。这篇文章总结了目前开发这种高保真端到端模型的工作状态,同时强调了它可能应用于地球辐射预算仪器。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
First-Principle Dynamic Electro-Thermal Numerical Model of a Scanning Radiometer for Earth Radiation Budget Applications
Earth Observing instruments that are used to monitor the incoming solar and outgoing longwave radiation from low-Earth orbit, have been a crucial part of studying the Earth's radiation budget during the past three decades. Instruments such as these go through several robust design phases followed by vigorous ground calibration campaigns to set their baseline characterization spectrally, spatially, temporally and radiometrically. The knowledge gained from building and calibrating these instruments has aided in technology advancements as the need for developing more accurate instruments has increased. In order to understand the instrument prelaunch performance, NASA Langley Research Center has partnered with the Thermal Radiation Group at Virginia Tech to develop a first-principle, dynamic electro-thermal, numerical model of a scanning radiometer that can be used to enhance the interpretation of an Earth radiation budget-like instrument on orbit. This contribution summarizes the current state of efforts to develop this high-fidelity end-to-end model and while highlighting its possible application to an Earth radiation budget instrument.
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