Abstract
Abstract. Reducing methane emissions is essential to tackle climate change. Here, we address the problem of detecting large methane leaks using hyperspectral data from the Sentinel-5P satellite. For that we exploit the fine spectral sampling of Sentinel-5P data to detect methane absorption features visible in the shortwave infrared wavelength range (SWIR). Our method involves three separate steps: i) background subtraction, ii) detection of local maxima in the negative logarithmic spectrum of each pixel and iii) anomaly detection in the background-free image. In the first step, we remove the impact of the albedo using albedo maps and the impact of the atmosphere by using a principal component analysis (PCA) over a time series of past observations. In the second step, we count for each pixel the number of local maxima that correspond to a subset of local maxima in the methane absorption spectrum. This counting method allows us to set up a statistical a contrario test that controls the false alarm rate of our detections. In the last step we use an anomaly detector to isolate potential methane plumes and we intersect those potential plumes with what have been detected in the second step. This process strongly reduces the number of false alarms. We validate our method by comparing the detected plumes against a dataset of plumes manually annotated on the Sentinel-5P L2 methane product.
Highlights
The detection of large methane (CH4) leaks linked to oil and gas production is currently a major stake in order to reduce greenhouse gas (GHG) emissions
Our objective is to introduce a flexible CH4 emission detection method using the level 1 (L1) data provided by Sentinel5P
In that way we reduce considerably the false alarms and obtain a proof that the methane fingerprint is present in the pixel after background subtraction
Summary
The detection of large methane (CH4) leaks linked to oil and gas production is currently a major stake in order to reduce greenhouse gas (GHG) emissions. Data from Sentinel-5P is publicly available and is already being used by ESA to quantify CH4 emissions and other greenhouse gases (Pandey et al, 2019). In order to detect potential local excess of CH4, we start by performing a background subtraction. It removes the contribution of albedo and atmosphere from the spectrum of the current pixel. It sets the mean CH4 concentration to zero.
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More From: ISPRS Annals of the Photogrammetry, Remote Sensing and Spatial Information Sciences
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