Abstract

The Sentinel-2 (S2) constellation provides multispectral images at 10 m, 20 m, and 60 m resolution bands. Obtaining all bands at 10 m resolution would benefit many applications. Recently, many model-based and deep learning (DL)-based sharpening methods have been proposed. However, the downside of those methods is that the DL-based methods need to be trained separately for the 20 m and the 60 m bands in a supervised manner at reduced resolution, while the model-based methods heavily depend on the hand-crafted image priors. To break the gap, this article proposes a novel unsupervised DL-based S2 sharpening method using a single convolutional neural network (CNN) to sharpen the 20 and 60 m bands at the same time at full resolution. The proposed method replaces the hand-crafted image prior by the deep image prior (DIP) provided by a CNN structure whose parameters are easily optimized using a DL optimizer. We also incorporate the modulation transfer function-based degradation model as a network layer, and add all bands to both network input and output. This setting improves the DIP and exploits the advantage of multitask learning since all S2 bands are highly correlated. Extensive experiments with real S2 data show that our proposed method outperforms competitive methods for reduced-resolution evaluation and yields very high quality sharpened image for full-resolution evaluation.

Highlights

  • M ULTISPECTRAL (MS) images provided by optical remote sensing imaging systems are needed in many applications, such as vegetation and water mapping [1], [2], crop monitoring [3], object classification [4], and many more

  • To break the gap between model-based and deep learning (DL)-based methods, we propose an unsupervised DL-based method, called S2SUCNN, which stands for Sentinel-2 sharpening using unsupervised convolutional neural network

  • The S2 constellations provide data in terms of tiles, where each tile covers an area of approximately 110 × 110 km2

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Summary

Introduction

M ULTISPECTRAL (MS) images provided by optical remote sensing imaging systems are needed in many applications, such as vegetation and water mapping [1], [2], crop monitoring [3], object classification [4], and many more. The MS images acquired by such systems often have one (or more) high spatial resolution (HR), wide spectral band(s), and some low spatial resolution (LR), narrow spectral bands. This is because of the hardware constraints, the limitations of data storage and transmission, and the preservation of image quality (e.g., signal-to-noise ratio)

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