We review progress, since publication of the book``Collisional effects on molecular spectra: Laboratory experiments and models, consequences for applications"(Elsevier, Amsterdam …
M Dammann, R Weber, A Fateev, S Clausen… - Journal of Quantitative …, 2024 - Elsevier
Line-by-line models based on spectroscopic databases are powerful tools for the generation of accurate gas absorption spectra but still require validation for high-temperature and high …
S Lebonnois, G Schubert - Nature Geoscience, 2017 - nature.com
With temperatures around 700 K and pressures of around 75 bar, the deepest 12 km of the atmosphere of Venus are so hot and dense that the atmosphere behaves like a supercritical …
The goal of this white paper is to provide a snapshot of the data availability and data needs primarily for the Ariel space mission, but also for related atmospheric studies of exoplanets …
During accretion, the young rocky planets are so hot that they become endowed with a magma ocean. From that moment, the mantle convective thermal flux control the cooling of …
The origin of the presence of geological and mineralogical evidence that liquid water flowed on the surface of early Mars is now a 50-year-old mystery. It has been proposed (Segura et …
Large planetesimals and planetary embryos ranging from several hundred to a few thousand kilometers can develop magma oceans through mutual collisions, gravitational …
S Lebonnois, V Eymet, C Lee… - Journal of Geophysical …, 2015 - Wiley Online Library
A detailed one‐dimensional analysis of the energy balance in Venus atmosphere is proposed in this work, based on the Net Exchange Rate formalism that allows the …
B Hu, Y Huang, X Liu, J Han, W Liu, M Xu - Energy & Fuels, 2025 - ACS Publications
The massive emission of carbon dioxide (CO2) has caused serious climate problems. Nondispersive infrared (NDIR) spectroscopy is a commonly used technique for CO2 …