Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Maria Zamyatina"'
Autor:
Jake Taylor, Michael Radica, Luis Welbanks, Ryan J MacDonald, Jasmina Blecic, Maria Zamyatina, Alexander Roth, Jacob L Bean, Vivien Parmentier, Louis-Philippe Coulombe, Adina D Feinstein, Néstor Espinoza, Bjórn Benneke, David Lafrenière, René Doyon, Eva-Maria Ahrer
The newly operational JWST offers the potential to study the atmospheres of distant worlds with precision that has not been achieved before. One of the first exoplanets observed by JWST in the summer of 2022 was WASP-96 b, a hot-Saturn orbiting a G8
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b605d4084350df89eb50d0458e9f4627
Autor:
Maria Zamyatina, Eric Hébrard, Benjamin Drummond, Nathan J Mayne, James Manners, Duncan A Christie, Pascal Tremblin, David K Sing, Krisztian Kohary
Transport-induced quenching, i.e., the homogenisation of chemical abundances by atmospheric advection, is thought to occur in the atmospheres of hot gas giant exoplanets. While some numerical modelling of this process exists, the three-dimensional na
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::19b1b74c1d8b0ab85743890e4ccf242c
http://arxiv.org/abs/2211.09071
http://arxiv.org/abs/2211.09071
Autor:
Marrick Braam, Paul I Palmer, Leen Decin, Robert J Ridgway, Maria Zamyatina, Nathan J Mayne, Denis E Sergeev, N Luke Abraham
Publikováno v:
Braam, M, Palmer, P I, Decin, L, Ridgway, R J, Zamyatina, M, Mayne, N J, Sergeev, D E & Abraham, N L 2022, ' Lightning-induced chemistry on tidally-locked Earth-like exoplanets ', Monthly Notices of the Royal Astronomical Society, vol. 517, no. 2, pp. 2383–2402 . https://doi.org/10.1093/mnras/stac2722
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::75d1bc0baae4ec6e5f0673e31c2beab8
https://hdl.handle.net/20.500.11820/f98643df-ed84-4fa3-b543-f918282fb409
https://hdl.handle.net/20.500.11820/f98643df-ed84-4fa3-b543-f918282fb409
Autor:
Duncan A. Christie, Elspeth K. H. Lee, Hamish Innes, Pascal A. Noti, Benjamin Charnay, Thomas J. Fauchez, Nathan J. Mayne, Russell Deitrick, Feng Ding, Jennifer J. Greco, Mark Hammond, Isaac Malsky, Avi Mandell, Emily Rauscher, Michael T. Roman, Denis E. Sergeev, Linda Sohl, Maria E. Steinrueck, Martin Turbet, Eric T. Wolf, Maria Zamyatina, Ludmila Carone
Publikováno v:
Christie, Duncan A.; Lee, Elspeth K. H.; Innes, Hamish; Noti, Pascal A.; Charnay, Benjamin; Fauchez, Thomas J.; Mayne, Nathan J.; Deitrick, Russell; Ding, Feng; Greco, Jennifer J.; Hammond, Mark; Malsky, Isaac; Mandell, Avi; Rauscher, Emily; Roman, Michael T.; Sergeev, Denis E.; Sohl, Linda; Steinrueck, Maria E.; Turbet, Martin; Wolf, Eric T.; ... (2022). CAMEMBERT: A Mini-Neptunes General Circulation Model Intercomparison, Protocol Version 1.0.A CUISINES Model Intercomparison Project. The planetary science journal, 3(11), p. 261. IOP Publishing 10.3847/PSJ/ac9dfe
With an increased focus on the observing and modeling of mini-Neptunes, there comes a need to better understand the tools we use to model their atmospheres. In this Paper, we present the protocol for the Comparing Atmospheric Models of Extrasolar Min
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3178a2201110ad828725f0bb6953e261
https://doi.org/10.3847/psj/ac9dfe
https://doi.org/10.3847/psj/ac9dfe
We present results from a set of cloud-free simulations of exoplanet atmospheres using a coupled three-dimensional (3D) hydrodynamics-radiation-chemistry model. We report in particular our investigation of the thermodynamic and chemical structure of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c595e30e1e72f7b203e861191ac44d04
https://doi.org/10.5194/epsc2021-573
https://doi.org/10.5194/epsc2021-573