Recent advances in collisional effects on spectra of molecular gases and their practical consequences
We review progress, since publication of the book``Collisional effects on molecular spectra:
Laboratory experiments and models, consequences for applications"(Elsevier, Amsterdam …
Laboratory experiments and models, consequences for applications"(Elsevier, Amsterdam …
Composition and chemistry of the neutral atmosphere of Venus
E Marcq, FP Mills, CD Parkinson, AC Vandaele - Space Science Reviews, 2018 - Springer
This paper deals with the composition and chemical processes occurring in the neutral
atmosphere of Venus. Since the last synthesis, observers as well as modellers have …
atmosphere of Venus. Since the last synthesis, observers as well as modellers have …
[图书][B] Collisional effects on molecular spectra: laboratory experiments and models, consequences for applications
JM Hartmann, C Boulet, D Robert - 2021 - books.google.com
Gas phase molecular spectroscopy is a powerful tool for obtaining information on the
geometry and internal structure of isolated molecules and their interactions with others. It …
geometry and internal structure of isolated molecules and their interactions with others. It …
Spatially resolved measurements of H2O, HCl, CO, OCS, SO2, cloud opacity, and acid concentration in the Venus near‐infrared spectral windows
We observed Venus with the Apache Point Observatory 3.5 m telescope TripleSpec
spectrograph (R= 3500, λ= 0.96–2.47 µm) on 1–3 March 2009 and on 25, 27, and 30 …
spectrograph (R= 3500, λ= 0.96–2.47 µm) on 1–3 March 2009 and on 25, 27, and 30 …
Scientific goals for the observation of Venus by VIRTIS on ESA/Venus Express mission
The Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on board the ESA/Venus
Express mission has technical specifications well suited for many science objectives of …
Express mission has technical specifications well suited for many science objectives of …
Infrared collision-induced and far-line absorption in dense CO2 atmospheres
R Wordsworth, F Forget, V Eymet - Icarus, 2010 - Elsevier
Collision-induced absorption is of great importance to the overall radiative budget in dense
CO2-rich atmospheres, but its representation in climate models remains uncertain, mainly …
CO2-rich atmospheres, but its representation in climate models remains uncertain, mainly …
The 1.10-and 1.18-μm nightside windows of Venus observed by SPICAV-IR aboard Venus Express
B Bézard, A Fedorova, JL Bertaux, A Rodin, O Korablev - Icarus, 2011 - Elsevier
Observations of the 1.10-and 1.18-μm nightside windows by the SPICAV-IR instrument
aboard Venus Express were analyzed to characterize the various sources of gaseous …
aboard Venus Express were analyzed to characterize the various sources of gaseous …
Consistently simulating a wide range of atmospheric scenarios for k2-18b with a flexible radiative transfer module
M Scheucher, F Wunderlich, JL Grenfell… - The Astrophysical …, 2020 - iopscience.iop.org
The atmospheres of small, potentially rocky exoplanets are expected to cover a diverse
range in composition and mass. Studying such objects therefore requires flexible and wide …
range in composition and mass. Studying such objects therefore requires flexible and wide …
Radiative heating and cooling in the middle and lower atmosphere of Venus and responses to atmospheric and spectroscopic parameter variations
R Haus, D Kappel, G Arnold - Planetary and Space Science, 2015 - Elsevier
A sophisticated radiative transfer model that considers absorption, emission, and multiple
scattering by gaseous and particulate constituents over the broad spectral range 0.125 …
scattering by gaseous and particulate constituents over the broad spectral range 0.125 …
Measurements and modelling of high pressure pure CO2 spectra from 750 to 8500 cm− 1. I—central and wing regions of the allowed vibrational bands
Precise modelling of infrared absorption by carbon dioxide is of primary importance for
radiative transfer calculations in CO2-rich atmospheres like those of Venus and Mars …
radiative transfer calculations in CO2-rich atmospheres like those of Venus and Mars …