An update on the RTTOV fast radiative transfer model (currently at version 12)
R Saunders, J Hocking, E Turner… - Geoscientific Model …, 2018 - gmd.copernicus.org
This paper gives an update of the RTTOV (Radiative Transfer for TOVS) fast radiative
transfer model, which is widely used in the satellite retrieval and data assimilation …
transfer model, which is widely used in the satellite retrieval and data assimilation …
The HITRAN2012 molecular spectroscopic database
LS Rothman, IE Gordon, Y Babikov, A Barbe… - Journal of Quantitative …, 2013 - Elsevier
This paper describes the status of the 2012 edition of the HITRAN molecular spectroscopic
compilation. The new edition replaces the previous HITRAN edition of 2008 and its updates …
compilation. The new edition replaces the previous HITRAN edition of 2008 and its updates …
The 2015 edition of the GEISA spectroscopic database
N Jacquinet-Husson, R Armante, NA Scott… - Journal of Molecular …, 2016 - Elsevier
The GEISA database (Gestion et Etude des Informations Spectroscopiques Atmosphériques:
Management and Study of Atmospheric Spectroscopic Information) has been developed …
Management and Study of Atmospheric Spectroscopic Information) has been developed …
New analytical model for the ozone electronic ground state potential surface and accurate ab initio vibrational predictions at high energy range
VG Tyuterev, RV Kochanov, SA Tashkun… - The Journal of …, 2013 - pubs.aip.org
An accurate description of the complicated shape of the potential energy surface (PES) and
that of the highly excited vibration states is of crucial importance for various unsolved issues …
that of the highly excited vibration states is of crucial importance for various unsolved issues …
[HTML][HTML] Version 8 IMK–IAA MIPAS temperatures from 12–15 µ m spectra: Middle and Upper Atmosphere modes
M García-Comas, B Funke… - Atmospheric …, 2023 - amt.copernicus.org
Motivated by an improved European Space Agency (ESA) version of calibrated Michelson
Interferometer for Passive Atmospheric Sounding (MIPAS) spectra (version 8.03), we have …
Interferometer for Passive Atmospheric Sounding (MIPAS) spectra (version 8.03), we have …
High accuracy molecular line lists for studies of exoplanets and other hot atmospheres
J Tennyson, SN Yurchenko - Frontiers in Astronomy and Space …, 2022 - frontiersin.org
The desire to characterize and model the atmospheres of the many extrasolar planets that
have been discovered over the last three decades is a major driver of current astronomy …
have been discovered over the last three decades is a major driver of current astronomy …
Mesospheric and stratospheric NOy produced by energetic particle precipitation during 2002–2012
B Funke, M López‐Puertas, GP Stiller… - Journal of …, 2014 - Wiley Online Library
Global distributions of the six principal reactive nitrogen (NOy) compounds (HNO3, NO2,
NO, N2O5, ClONO2, and HNO4) have been derived from midinfrared limb emission spectra …
NO, N2O5, ClONO2, and HNO4) have been derived from midinfrared limb emission spectra …
S&MPO–An information system for ozone spectroscopy on the WEB
YL Babikov, SN Mikhailenko, A Barbe… - Journal of Quantitative …, 2014 - Elsevier
Abstract Spectroscopy and Molecular Properties of Ozone (“S&MPO”) is an Internet
accessible information system devoted to high resolution spectroscopy of the ozone …
accessible information system devoted to high resolution spectroscopy of the ozone …
Detection and assignment of ozone bands near 95% of the dissociation threshold: Ultrasensitive experiments for probing potential energy function and vibrational …
S Vasilchenko, A Barbe, E Starikova, S Kassi… - Physical Review A, 2020 - APS
Ozone formation and depletion play a key role in various physical and chemical atmospheric
processes which remain to be understood in more detail. The modeling of such phenomena …
processes which remain to be understood in more detail. The modeling of such phenomena …
HEPPA-II model-measurement intercomparison project: EPP indirect effects during the dynamically perturbed NH winter 2008–2009
We compare simulations from three high-top (with upper lid above 120 km) and five medium-
top (with upper lid around 80km) atmospheric models with observations of odd nitrogen (NO …
top (with upper lid around 80km) atmospheric models with observations of odd nitrogen (NO …