Machine learning for automatic identification of new minor species

DOI: 
10.1016/j.jqsrt.2020.107361
Publication date: 
01/01/2021
Main author: 
Schmidt F.
IAA authors: 
Lopez-Moreno, Jose Juan
Authors: 
Schmidt, Frédéric;Mermy, Guillaume Cruz;Erwin, Justin;Robert, Séverine;Neary, Lori;Thomas, Ian R.;Daerden, Frank;Ristic, Bojan;Patel, Manish R.;Bellucci, Giancarlo;Lopez-Moreno, Jose Juan;Vandaele, Ann Carine
Journal: 
Journal of Quantitative Spectroscopy and Radiative Transfer
Refereed: 
Yes
Publication type: 
Article
Volume: 
259
Pages: 
107361
Number: 
107361
Abstract: 
© 2020 One of the main difficulties to analyze modern spectroscopic datasets is due to the large amount of data. For example, in atmospheric transmittance spectroscopy, the solar occultation channel (SO) of the NOMAD instrument onboard the ESA ExoMars2016 satellite called Trace Gas Orbiter (TGO) had produced ~ 10 millions of spectra in ~ 20000 acquisition sequences since the beginning of the mission in April 2018 until 15 January 2020. Other datasets are even larger with ~ billions of spectra for OMEGA onboard Mars Express or CRISM onboard Mars Reconnaissance Orbiter. Usually, new lines are discovered after a long iterative process of model fitting and manual residual analysis. Here we propose a new method based on unsupervised machine learning, to automatically detect new minor species. Although precise quantification is out of scope, this tool can also be used to quickly summarize the dataset, by giving few endmembers (”source”) and their abundances. The methodology is the following: we proposed a way to approximate the dataset non-linearity by a linear mixture of abundance and source spectra (endmembers). We used unsupervised source separation in form of non-negative matrix factorization to estimate those quantities. Several methods are tested on synthetic and simulation data. Our approach is dedicated to detect minor species spectra rather than precisely quantifying them. On synthetic example, this approach is able to detect chemical compounds present in form of 100 hidden spectra out of 104, at 1.5 times the noise level. Results on simulated spectra of NOMAD-SO targeting CH4 show that detection limits goes in the range of 100–500 ppt in favorable conditions. Results on real martian data from NOMAD-SO show that CO2 and H2O are present, as expected, but CH4 is absent. Nevertheless, we confirm a set of new unexpected lines in the database, attributed by ACS instrument Team to the CO2 magnetic dipole.
Database: 
SCOPUS
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2021JQSRT.25907361S/abstract
ADS Bibcode: 
2021JQSRT.25907361S
Keywords: 
Atmosphere | Data mining | Machine learning | Non-negative matrix factorization | Source separation | Spectroscopy | Unsupervised