D'Odorico Petra, Alberti Edoardo, Schaepman Michael E
Remote Sensing Laboratories, University of Zurich, Winterthurerstrasse 190, CH-8057 Zurich, Switzerland.
Appl Opt. 2010 Jun 1;49(16):3082-91. doi: 10.1364/AO.49.003082.
Spectral performance of an airborne dispersive pushbroom imaging spectrometer cannot be assumed to be stable over a whole flight season given the environmental stresses present during flight. Spectral performance monitoring during flight is commonly accomplished by looking at selected absorption features present in the Sun, atmosphere, or ground, and their stability. The assessment of instrument performance in two different environments, e.g., laboratory and airborne, using precisely the same calibration reference, has not been possible so far. The Airborne Prism Experiment (APEX), an airborne dispersive pushbroom imaging spectrometer, uses an onboard in-flight characterization (IFC) facility, which makes it possible to monitor the sensor's performance in terms of spectral, radiometric, and geometric stability in flight and in the laboratory. We discuss in detail a new method for the monitoring of spectral instrument performance. The method relies on the monitoring of spectral shifts by comparing instrument-induced movements of absorption features on ground and in flight. Absorption lines originate from spectral filters, which intercept the full field of view (FOV) illuminated using an internal light source. A feature-fitting algorithm is used for the shift estimation based on Pearson's correlation coefficient. Environmental parameter monitoring, coregistered on board with the image and calibration data, revealed that differential pressure and temperature in the baffle compartment are the main driving parameters explaining the trend in spectral performance deviations in the time and the space (across-track) domains, respectively. The results presented in this paper show that the system in its current setup needs further improvements to reach a stable performance. Findings provided useful guidelines for the instrument revision currently under way. The main aim of the revision is the stabilization of the instrument for a range of temperature and pressure conditions to be encountered during operation.
鉴于飞行过程中存在的环境压力,不能假定机载色散推扫式成像光谱仪的光谱性能在整个飞行季节都是稳定的。飞行过程中的光谱性能监测通常是通过观察太阳、大气或地面中存在的选定吸收特征及其稳定性来完成的。到目前为止,使用完全相同的校准参考来评估仪器在两种不同环境(例如实验室和机载环境)中的性能是不可能的。机载棱镜实验(APEX)是一种机载色散推扫式成像光谱仪,它使用机载飞行中特性描述(IFC)设施,这使得在飞行中和实验室中监测传感器在光谱、辐射和几何稳定性方面的性能成为可能。我们详细讨论了一种监测光谱仪器性能的新方法。该方法依赖于通过比较地面和飞行中吸收特征的仪器诱导移动来监测光谱偏移。吸收线源自光谱滤光片,这些滤光片拦截使用内部光源照亮的全视场(FOV)。基于皮尔逊相关系数,使用特征拟合算法进行偏移估计。与图像和校准数据一起在机载上进行的环境参数监测表明,挡板隔舱中的压差和温度分别是解释时间域和空间(沿轨)域光谱性能偏差趋势的主要驱动参数。本文给出的结果表明,该系统目前的设置需要进一步改进以达到稳定的性能。研究结果为正在进行的仪器修订提供了有用的指导方针。修订的主要目标是使仪器在运行过程中遇到的一系列温度和压力条件下保持稳定。