Zobrazeno 1 - 10
of 459
pro vyhledávání: '"PALMER, PAUL I."'
Autor:
Martínez, Francisco Ardévol, Min, Michiel, Huppenkothen, Daniela, Kamp, Inga, Palmer, Paul I.
Interpreting the observations of exoplanet atmospheres to constrain physical and chemical properties is typically done using Bayesian retrieval techniques. Because these methods require many model computations, a compromise is made between model comp
Externí odkaz:
http://arxiv.org/abs/2401.04168
Haze optical depth in exoplanet atmospheres varies with rotation rate: Implications for observations
Transmission spectroscopy supports the presence of uncharacterised, light-scattering and -absorbing aerosols in the atmospheres of many exoplanets. The complexity of factors influencing the formation, 3-D transport, radiative impact, and removal of a
Externí odkaz:
http://arxiv.org/abs/2307.10931
Publikováno v:
MNRAS, 526, 1 (2023)
Determining the habitability and interpreting future atmospheric observations of exoplanets requires understanding the atmospheric dynamics and chemistry from a 3-D perspective. Previous studies have shown significant spatial variability in the ozone
Externí odkaz:
http://arxiv.org/abs/2306.03004
Autor:
Whiteford, Niall, Glasse, Alistair, Chubb, Katy L., Kitzmann, Daniel, Ray, Shrishmoy, Phillips, Mark W., Biller, Beth A., Palmer, Paul I., Rice, Ken, Waldmann, Ingo P., Changeat, Quentin, Skaf, Nour, Wang, Jason, Edwards, Billy, Al-Refaie, Ahmed
Retrieval methods are a powerful analysis technique for modelling exoplanetary atmospheres by estimating the bulk physical and chemical properties that combine in a forward model to best-fit an observed spectrum, and they are increasingly being appli
Externí odkaz:
http://arxiv.org/abs/2302.07939
Publikováno v:
Planet. Sci. J. 4 68 (2023)
Cloud cover at the planetary limb of water-rich Earth-like planets is likely to weaken chemical signatures in transmission spectra, impeding attempts to characterize these atmospheres. However, based on observations of Earth and solar system worlds,
Externí odkaz:
http://arxiv.org/abs/2211.11887
Autor:
Ridgway, Robert J., Zamyatina, Maria, Mayne, Nathan J., Manners, James, Lambert, F. Hugo, Braam, Marrick, Drummond, Benjamin, Hébrard, Éric, Palmer, Paul I., Kohary, Krisztian
Stellar flares present challenges to the potential habitability of terrestrial planets orbiting M dwarf stars through inducing changes in the atmospheric composition and irradiating the planet's surface in large amounts of ultraviolet light. To exami
Externí odkaz:
http://arxiv.org/abs/2210.13257
Autor:
Braam, Marrick, Palmer, Paul I., Decin, Leen, Ridgway, Robert J., Zamyatina, Maria, Mayne, Nathan J., Sergeev, Denis E., Abraham, N. Luke
Determining the habitability and interpreting atmospheric spectra of exoplanets requires understanding their atmospheric physics and chemistry. We use a 3-D Coupled Climate-Chemistry Model, the Met Office Unified Model with the UK Chemistry and Aeros
Externí odkaz:
http://arxiv.org/abs/2209.12502
Publikováno v:
A&A 662, A108 (2022)
Exoplanet observations are currently analysed with Bayesian retrieval techniques. Due to the computational load of the models used, a compromise is needed between model complexity and computing time. Analysis of data from future facilities, will need
Externí odkaz:
http://arxiv.org/abs/2203.01236