A. Perrin

ORCID: 0000-0003-0662-3973
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About
Contact & Profiles
Research Areas
  • Spectroscopy and Laser Applications
  • Atmospheric Ozone and Climate
  • Atmospheric and Environmental Gas Dynamics
  • Atmospheric chemistry and aerosols
  • Advanced Chemical Physics Studies
  • Molecular Spectroscopy and Structure
  • Calibration and Measurement Techniques
  • Inorganic Fluorides and Related Compounds
  • Water Quality Monitoring and Analysis
  • Phase Equilibria and Thermodynamics
  • Electron Spin Resonance Studies
  • Astrophysics and Star Formation Studies
  • Spectroscopy and Quantum Chemical Studies
  • Analytical Chemistry and Chromatography
  • Advanced NMR Techniques and Applications
  • Chemical Thermodynamics and Molecular Structure
  • Atmospheric aerosols and clouds
  • Advanced Chemical Sensor Technologies
  • Spectroscopy Techniques in Biomedical and Chemical Research
  • Radiation Detection and Scintillator Technologies
  • ZnO doping and properties
  • Air Quality Monitoring and Forecasting
  • Renal function and acid-base balance
  • Luminescence Properties of Advanced Materials
  • Porphyrin and Phthalocyanine Chemistry

Université Paris-Saclay
2018-2024

École Polytechnique
2018-2024

Centre National de la Recherche Scientifique
2009-2024

Laboratoire de Météorologie Dynamique
2018-2024

École Normale Supérieure - PSL
2023

Sorbonne Université
1990-2023

Université Paris Sciences et Lettres
2023

University of Cologne
2013-2021

James Madison University
2021

Planetary Systems (United States)
2021

This paper describes the contents of 2016 edition HITRAN molecular spectroscopic compilation. The new replaces previous 2012 and its updates during intervening years. absorption compilation is composed five major components: traditional line-by-line parameters required for high-resolution radiative-transfer codes, infrared cross-sections molecules not yet amenable to representation in a form, collision-induced data, aerosol indices refraction, general tables such as partition sums that apply...

10.1016/j.jqsrt.2017.06.038 article EN cc-by-nc-nd Journal of Quantitative Spectroscopy and Radiative Transfer 2017-07-05

The HITRAN database is a compilation of molecular spectroscopic parameters. It was established in the early 1970s and used by various computer codes to predict simulate transmission emission light gaseous media (with an emphasis on terrestrial planetary atmospheres). composed five major components: line-by-line parameters required for high-resolution radiative-transfer codes, experimental infrared absorption cross-sections (for molecules where it not yet feasible representation form),...

10.1016/j.jqsrt.2021.107949 article EN cc-by Journal of Quantitative Spectroscopy and Radiative Transfer 2021-09-27

Nineteen ninety-eight marks the 25th anniversary of release first HITRAN database. is recognized as international standard fundamental spectroscopic parameters for diverse atmospheric and laboratory transmission radiance calculations. There have been periodic editions over past decades database has expanded improved with respect to molecular species spectral range covered, number included, accuracy this information. The 1996 edition not only includes customary line-by-line transition...

10.1117/12.327146 article EN Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE 1998-07-07

Abstract. This article describes the latest stable release (version 2.2) of Atmospheric Radiative Transfer Simulator (ARTS), a public domain software for radiative transfer simulations in thermal spectral range (microwave to infrared). The main feature this is planetary toolbox that allows planets Venus, Mars, and Jupiter, addition Earth. required considerable model adaptations, most notably area gaseous absorption calculations. Other new features are also described, radio link budgets...

10.5194/gmd-11-1537-2018 article EN cc-by Geoscientific model development 2018-04-18

Very low-mass stars (those <0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars, but the compositions those are largely unknown. We use mid-infrared spectroscopy with James Webb Space Telescope to investigate chemical composition planet-forming disk around ISO-ChaI 147, a 0.11 solar-mass star. The inner has carbon-rich chemistry: we identify emission from 13 carbon-bearing molecules including ethane and benzene. derive large column densities...

10.1126/science.adi8147 article EN Science 2024-06-06

10.1016/j.jqsrt.2011.06.018 article EN Journal of Quantitative Spectroscopy and Radiative Transfer 2011-07-06
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