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Post Launch Calibration and Testing of The Geostationary Lightning Mapper on GOES-R Satellite

机译:发布推出校准和GoS-R卫星上的Geodationary Lightning Mapper的测试

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The Geostationary Operational Environmental Satellite R (GOES-R) series is the planned next generation of operational weather satellites for the United States National Oceanic and Atmospheric Administration (NOAA). The National Aeronautics and Space Administration (NASA) is procuring the GOES-R spacecraft and instruments with the first launch of the GOES-R series planned for October 2016. Included in the GOES-R Instrument suite is the Geostationary Lightning Mapper (GLM). GLM is a single-channel, near-infrared optical detector that can sense extremely brief (800 us) transient changes in the atmosphere, indicating the presence of lightning. GLM will measure total lightning activity continuously over the Americas and adjacent ocean regions with near-uniform spatial resolution of approximately 10 km. Due to its large CCD (1372×1300 pixels), high frame rate, sensitivity and onboard event filtering, GLM will require extensive post launch characterization and calibration. Daytime and nighttime images will be used to characterize both image quality criteria inherent to GLM as a space-based optic system (focus, stray light, crosstalk, solar glint) and programmable image processing criteria (dark offsets, gain, noise, linearity, dynamic range). In addition ground data filtering will be adjusted based on lightning-specific phenomenology (coherence) to isolate real from false transients with their own characteristics. These parameters will be updated, as needed, on orbit in an iterative process guided by pre-launch testing. This paper discusses the planned tests to be performed on GLM over the six-month Post Launch Test period to optimize and demonstrate GLM performance.
机译:地球静止运营环境卫星R(GOY-R)系列是美国国家海洋和大气管理局(NOAA)的下一代运营天气卫星。美国国家航空航天局(NASA)正在采购GoS-R航天器和仪器,并在2016年10月计划的GOY-R系列推出。GUS-R仪器套件中包含的是地静止闪电映射器(GLM)。 GLM是一个单通道,近红外光学探测器,可以在大气中感觉到极其简短的(800美元)的瞬态变化,表明存在闪电。 GLM将在美洲和邻近的海洋地区衡量总闪电活动,近均匀的空间分辨率约为10公里。由于其大CCD(1372×1300像素),高帧速率,灵敏度和板载滤波,GLM将需要大量发布发布表征和校准。白天和夜间图像将用于表征GLM固有的图像质量标准,作为基于空间的光学系统(焦点,杂散光,串扰,太阳闪光)和可编程图像处理标准(黑暗偏移,增益,噪声,线性,动态范围)。此外,基于闪电特定的现象学(一致性)来调整地面数据滤波,以利用自己的特性将真实瞬变隔离。根据需要,这些参数将根据需要在预启动测试引导的迭代过程中轨道上更新。本文讨论了在六个月后发射测试期间对GLM进行的计划测试,以优化和展示GLM性能。

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