基于字典和机器学习的光谱超分辨率高光谱图像重建

Swastik Bhattacharya, K. Remane, B. Kindel, Gongguo Tang
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引用次数: 1

摘要

高光谱传感器测量数百个波长通道的辐射光谱,分辨率通常在10nm左右,由全宽半最大值(FWHM)表示。光谱应用于生物、地质和海洋科学等表面材料的研究,利用定量光谱技术。由于频带数量的增加,为测量此类数据而开发的仪器价格昂贵,并且创建的大型数据集可能难以针对给定实例进行下行。星载地球表面高光谱观测的重复周期也比多光谱传感器少。发展具有成本效益并能产生预期结果的机制成为义不容辞的责任。为此,在机载可见光和红外成像光谱仪(AVIRIS)数据上尝试光谱超分辨率(SR),通过字典学习从等间隔的窄多光谱波段重建高光谱波段辐射,然后使用机器学习进行去噪。首先利用k -奇异值分解(K-SVD)训练的字典对30个输入的多光谱波段进行高光谱波段亮度估计,然后利用随机森林回归进行去噪。随机森林去噪后重建的总体信噪比(SNR)为31.58dB。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spectral Super-Resolution for Hyperspectral Image Reconstruction Using Dictionary and Machine Learning
Hyperspectral sensors measure the radiance spectrum across hundreds of wavelength channels with a resolution typically on the order of 10 nm represented by the full-width-half-maximum (FWHM). The spectra are used in the study of surface materials in the biological, geological and oceanographic sciences to name a few, utilizing quantitative spectroscopic techniques. The instruments developed to measure such data are expensive due to the increased number of bands, and create large datasets that can be difficult to downlink for a given instance. Repeat cycle of space-borne hyperspectral observations of the earth surface is also less than those of multi-spectral sensors. It becomes incumbent to develop mechanisms that could be cost-effective and give desired results. With this aim, spectral Super-Resolution (SR) is attempted on the Airborne Visible and Infra-Red Imaging Spectrometer (AVIRIS) data to reconstruct the hyperspectral band radiance from equally-spaced narrow multi-spectral bands using dictionary learning, followed by denoising using machine learning. The hyperspectral band radiance are first estimated from 30 selected input multi-spectral bands using dictionary trained through K-Singular Value Decomposition (K-SVD), followed by denoising using Random Forest Regression. An overall Signal-to-Noise Ratio (SNR) of 31.58dB is observed from reconstruction after denoising using Random Forest.
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