Sun Xiaoli, Abshire James B, Borsa Adrian A, Fricker Helen A, Yi Donghui, DiMarzio John P, Paolo Fernando S, Brunt Kelly M, Harding David J, Neumann Gregory A
Solar Exploration Division, National Aeronautic and Space Administration (NASA) Goddard Space Flight Center (GSFC), Greenbelt, MD 20771 USA (
Scripps Institution of Oceanography, University of California San Diego, La Jolla, CA 92093 USA.
IEEE Trans Geosci Remote Sens. 2017 Oct;55(10):5440-5454. doi: 10.1109/TGRS.2017.2702126. Epub 2017 Jul 25.
NASA's Ice, Cloud, and land Elevation Satellite (ICESat), which operated between 2003 and 2009, made the first satellite-based global lidar measurement of Earth's ice sheet elevations, sea-ice thickness and vegetation canopy structure. The primary instrument on ICESat was the Geoscience Laser Altimeter System (GLAS), which measured the distance from the spacecraft to Earth's surface via the roundtrip travel time of individual laser pulses. GLAS utilized pulsed lasers and a direct detection receiver consisting of a silicon avalanche photodiode (Si APD) and a waveform digitizer. Early in the mission, the peak power of the received signal from snow and ice surfaces was found to span a wider dynamic range than planned, often exceeding the linear dynamic range of the GLAS 1064-nm detector assembly. The resulting saturation of the receiver distorted the recorded signal and resulted in range biases as large as ~50 cm for ice and snow-covered surfaces. We developed a correction for this "saturation range bias" based on laboratory tests using a spare flight detector, and refined the correction by comparing GLAS elevation estimates to those derived from Global Positioning System (GPS) surveys over the calibration site at the salar de Uyuni, Bolivia. Applying the saturation correction largely eliminated the range bias due to receiver saturation for affected ICESat measurements over Uyuni and significantly reduced the discrepancies at orbit crossovers located on flat regions of the Antarctic ice sheet.
美国国家航空航天局的冰、云和陆地高程卫星(ICESat)于2003年至2009年运行,首次对地球冰盖高程、海冰厚度和植被冠层结构进行了基于卫星的全球激光雷达测量。ICESat上的主要仪器是地球科学激光高度计系统(GLAS),它通过单个激光脉冲的往返传播时间测量航天器到地球表面的距离。GLAS使用脉冲激光器和由硅雪崩光电二极管(Si APD)和波形数字化仪组成的直接探测接收器。在任务早期,发现来自冰雪表面的接收信号的峰值功率跨越的动态范围比计划的更宽,经常超过GLAS 1064纳米探测器组件的线性动态范围。接收器的饱和导致记录信号失真,并导致冰雪覆盖表面的距离偏差高达约50厘米。我们基于使用备用飞行探测器的实验室测试,开发了针对这种“饱和距离偏差”的校正方法,并通过将GLAS高程估计值与在玻利维亚乌尤尼盐沼校准地点的全球定位系统(GPS)测量得出的估计值进行比较,对校正方法进行了优化。应用饱和校正很大程度上消除了受影响的ICESat在乌尤尼上空测量时由于接收器饱和导致的距离偏差,并显著减少了位于南极冰盖平坦区域的轨道交叉点处的差异。