Guanter Luis, Segl Karl, Sang Bernhard, Alonso Luis, Kaufmann Hermann, Moreno Jose
Helmholtz Centre Potsdam GFZ German Research Centre For Geosciences, Telegrafenberg, D-14473 Potsdam, Germany.
Opt Express. 2009 Jul 6;17(14):11594-606. doi: 10.1364/oe.17.011594.
An accurate knowledge of the spectral calibration of imaging spectrometers is required for optimum data processing and interpretation. The scene-based spectral characterization of imaging spectrometers is frequently necessary to update or replace the pre-flight laboratory-based spectral characterization supplied by the data provider. An automatic method for the estimation of spectral calibration parameters (channel position and bandwidth) at atmospheric absorption regions from high spectral resolution imaging spectrometers (spectral sampling interval below 5 nm) is presented in this contribution. The method has been tested on two commercial instruments with spectral sampling intervals below 2.5 nm. Optical aberrations such as smile, spectrometer shift and rotation and degradation of channel bandwidth have been detected and are discussed in terms of potential error sources at the instrument level.
为了实现最佳的数据处理和解释,需要准确了解成像光谱仪的光谱校准。成像光谱仪基于场景的光谱特性描述通常是更新或替换数据提供商提供的飞行前基于实验室的光谱特性描述所必需的。本文提出了一种从高光谱分辨率成像光谱仪(光谱采样间隔低于5nm)估计大气吸收区域光谱校准参数(通道位置和带宽)的自动方法。该方法已在两台光谱采样间隔低于2.5nm的商业仪器上进行了测试。已检测到诸如微笑、光谱仪偏移和旋转等光学像差以及通道带宽的退化,并从仪器层面的潜在误差源角度进行了讨论。