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Improving Imaging Spectrometer Methane Plume Detection with Large Eddy Simulations
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  • Arjun Ashok Rao,
  • Steffen Mauceri,
  • Andrew Thorpe,
  • Jake Lee,
  • Siraput Jongaramrungruang,
  • Riley Duren
Arjun Ashok Rao
NASA Jet Propulsion Laboratory, NASA Jet Propulsion Laboratory

Corresponding Author:[email protected]

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Steffen Mauceri
NASA Jet Propulsion Laboratory, NASA Jet Propulsion Laboratory
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Andrew Thorpe
NASA Jet Propulsion Laboratory, NASA Jet Propulsion Laboratory
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Jake Lee
NASA Jet Propulsion Laboratory, NASA Jet Propulsion Laboratory
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Siraput Jongaramrungruang
California Institute of Technology, California Institute of Technology
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Riley Duren
University of Arizona, University of Arizona
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Abstract

Methane’s high heat trapping potential has made it a priority for quantification and mitigation efforts worldwide. Ground-based surveys and in-situ measurement techniques to quantify natural and fugitive methane emission sources are time-consuming, expensive, and often lead to sparse measurements. Failure to accurately quantify emissions at the point-source scale have thus led to poorly constrained emission estimates. Airborne imaging spectrometers such as the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS-NG) and the Global Airborne Observatory (GAO) have been employed to map the often stochastic and intermittent point-source emissions from a diverse set of source types including oil and gas, dairy, etc. A matched filter is applied to the methane-absorption relevant spectral features of the instrument’s radiance cube. Machine learning models are then trained to recognize methane plumes from these column-matched filter methane maps. However, current Convolutional Neural Network (CNN) models suffer from a high false-positive rate and poorly generalize to new scenes. False-positive detections are primarily due to methane absorption-mimicking surface spectroscopic features, as well as a lack of training data. To supplement the available training data, we utilize Large Eddy Simulations (LES) of methane point-source emissions to train a Convolutional Neural Network (CNN) on a plume-classification task. We observe a significant distribution shift between LES and AVIRIS-NG plumes, primarily caused by high LES plume enhancements. Through a series of image transforms verified through an adversarial approach using a discriminator network, we minimize the distribution shift between synthetic LES plumes and plumes observed by AVIRIS-NG and GAO. CNNs trained on a mixture of LES and real-world plumes, and tested on flightlines from multiple campaigns exhibit an error reduction compared to previous models. The reduction in false-positive plume detections demonstrates that supplementing the limited training data of real methane plumes with LES provides an avenue to make automatic detection more robust for future airborne and spaceborne missions such as SBG, EMIT, and Carbon Mapper.