Venus Evolution Through Time: Key Science Questions, Selected Mission Concepts and Future Investigations
Space Science Reviews Springer 219:7 (2023) 56
Abstract:
Collisional parameters of H2O with CO2 are currently missing from international spectroscopic databases, although they are essential for accurate modeling of water vapor in CO2-rich planetary atmospheres. In this study, high-resolution infrared spectra of H2O broadened by CO2 were recorded using a Fourier Transform Spectrometer in the 1.18 and 2.34 µm spectral regions. CO2-collisional parameters for selected H2O transitions were derived through a multispectrum fitting procedure employing both Voigt and quadratic speed-dependent Voigt profiles. Furthermore, calculations based on the semi-classical Complex Robert-Bonamy-Ma formalism were performed to estimate CO2-broadened half-widths, line shifts, and their temperature dependencies across various atmospheric transparency windows. It results in a strong agreement between theoretical predictions and experimental data. Finally, the shared calculated linelist, obtained for a wide range of transitions, can be directly applied to radiative transfer modeling of atmospheres primarily composed of carbon dioxidePreface for special issue on the Colour and Stereo Surface Imaging System (CaSSIS) at Mars
Planetary and Space Science Elsevier 236 (2023) 105753
Solar Energetic Particle Events Detected in the Housekeeping Data of the European Space Agency's Spacecraft Flotilla in the Solar System
Space Weather American Geophysical Union (AGU) 21:8 (2023)
The Habitability of Venus
Space Science Reviews Springer 219:2 (2023) 17
Abstract:
The conditions of the surface of Venus are extremely harsh, and there is no naturally evolved life on Venus. E. coli is a bacteria with a number of subtypes and adaptations to varying environments. This paper covers a number of adaptations a theoretical colony of E. coli bacteria could evolve, based on pre-existing adaptations of E. coli to its natural environmentsVenus, the Planet: Introduction to the Evolution of Earth’s Sister Planet
Space Science Reviews Springer 219:1 (2023) 10