DA
David Skålid Amundsen
astro-ph.EPastro-ph.SRphysics.class-phcond-mat.softModels, TheoreticalAquaplanetAtmosphereClimatecond-mat.mtrl-sciExoplanets
On Valency
published · living versionsW_nyrwa6jm·v1 · currentpublished
Accuracy tests of radiation schemes used in hot Jupiter global circulation models
with Isabelle Baraffe, Pascal Tremblin, James Manners, Wolfgang Hayek +2
1 version
W_q2fxenbq·v1published
W_ukx56v5a·v1published
Preprints & journals
28 papers in the corpus · 2011–2023A mixed local and nonlocal supercritical Dirichlet problems2303.03273v4 · David Amundsen, Abbas Moameni, Remi Yvant Temgoua2023 · 0 citationsarXiv
Minimal model for slow, sub-Rayleigh, supershear, and unsteady rupture propagation along homogeneously loaded frictional interfaces.31771025 · Thøgersen, Kjetil, Sveinsson, Henrik Andersen, Amundsen, David Skålid et al.2019 · 3 citationsPhysical review. E. 2019;100(4-1):043004
Habitable Climate Scenarios for Proxima Centauri b with a Dynamic Ocean.30183335 · Del Genio, Anthony D, Way, Michael J, Amundsen, David S et al.2020 · 125 citationsAstrobiology. 2019;19(1):99-125
Simulating the cloudy atmospheres of HD 209458 b and HD 189733 b with the 3D Met Office Unified Model1803.00226v1 · S. Lines, N. J. Mayne, Ian A. Boutle et al.2018 · 109 citationsA&A 615, A97 (2018)
Modeling Venus-Like Worlds Through Time1802.05434v1 · M.J. Way, Anthony Del Genio, David S. Amundsen2018 · 2 citationsarXiv
The effect of metallicity on the atmospheres of exoplanets with fully coupled 3D hydrodynamics, equilibrium chemistry, and radiative transfer1801.01045v1 · Benjamin Drummond, N. J. Mayne, Isabelle Baraffe et al.2018 · 65 citationsarXiv
A library of ATMO forward model transmission spectra for hot Jupiter exoplanets1710.10269v4 · Jayesh M. Goyal, Nathan Mayne, David K. Sing et al.2017 · 122 citationsMonthly Notices of the Royal Astronomical Society, Volume 474, Issue 4, March 2018, Pages 5158-5185
An ultrahot gas-giant exoplanet with a stratosphere.28770846 · Evans, Thomas M, Sing, David K, Kataria, Tiffany et al.2017 · 262 citationsNature. 2017;548(7665):58-61
NIR-Driven Moist Upper Atmospheres of Synchronously Rotating Temperate Terrestrial Exoplanets1704.05878v2 · Yuka Fujii, Anthony D. Del Genio, David S. Amundsen2017 · 70 citationsAstrophysical Journal, 848, 100 (2017)
Advection of potential temperature in the atmosphere of irradiated exoplanets: a robust mechanism to explain radius inflation1704.05440v1 · P. Tremblin, G. Chabrier, N. J. Mayne et al.2017 · 146 citationsarXiv
Results from a set of three-dimensional numerical experiments of a hot Jupiter atmosphere1704.00539v1 · N. J. Mayne, F. Debras, I. Baraffe et al.2017 · 70 citationsA&A 604, A79 (2017)
Parallaxes and Infrared Photometry of three Y0 dwarfs1703.10341v1 · R. L. Smart, D'aniel Apai, J. Davy Kirkpatrick et al.2017 · 8 citationsarXiv
Resolving Orbital and Climate Keys of Earth and Extraterrestrial Environments with Dynamics 1.0: A General Circulation Model for Simulating the Climates of Rocky Planets1701.02360v2 · M. J. Way, Igor Aleinov, David. S. Amundsen et al.2017 · 127 citationsarXiv
Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models1610.01389v1 · David S. Amundsen, Pascal Tremblin, James Manners et al.2016 · 138 citationsA&A 598, A97 (2017)on Valency
The Effects of Consistent Chemical Kinetics Calculations on the Pressure-Temperature Profiles and Emission Spectra of Hot Jupiters1607.04062v1 · Benjamin Drummond, Pascal Tremblin, Isabelle Baraffe et al.2016 · 170 citationsarXiv
Detection of H2O and evidence for TiO/VO in an ultra hot exoplanet atmosphere1604.02310v1 · Thomas M. Evans, David K. Sing, Hannah R. Wakeford et al.2016 · 226 citationsarXivon Valency
Near-Infrared Spectroscopy of the Y0 WISEP J173835.52+273258.9 and the Y1 WISE J035000.32-565830.2: the Importance of Non-Equilibrium Chemistry1603.09400v1 · S. K. Leggett, P. Tremblin, D. Saumon et al.2016 · 30 citationsarXiv
The mineral clouds on HD 209458b and HD189733b1603.04022v4 · Ch. Helling, G. Lee, I. Dobbs-Dixon et al.2016 · 98 citationsarXiv
The Need for Laboratory Work to Aid in The Understanding of Exoplanetary Atmospheres1602.06305v2 · Jonathan J. Fortney, Tyler D. Robinson, Shawn Domagal-Goldman et al.2016 · 33 citationsarXiv
Cloudless atmospheres for L/T dwarfs and extra-solar giant planets1601.03652v1 · P. Tremblin, D. S. Amundsen, G. Chabrier et al.2016 · 190 citationsarXiv
Steady-state propagation speed of rupture fronts along one-dimensional frictional interfaces.26465481 · Amundsen, David Skålid, Trømborg, Jørgen Kjoshagen, Thøgersen, Kjetil et al.2016 · 17 citationsPhysical review. E, Statistical, nonlinear, and soft matter physics. 2015;92(3):032406
A uniform analysis of HD209458b Spitzer/IRAC lightcurves with Gaussian process models1504.05942v1 · Thomas M. Evans, Suzanne Aigrain, Neale Gibson et al.2015 · 128 citationsarXiv
Fingering convection and cloudless models for cool brown dwarf atmospheres1504.03334v1 · P. Tremblin, D. S. Amundsen, P. Mourier et al.2015 · 271 citationsarXiv
Slow slip and the transition from fast to slow fronts in the rupture of frictional interfaces.24889640 · Trømborg, Jørgen Kjoshagen, Sveinsson, Henrik Andersen, Scheibert, Julien et al.2014 · 55 citationsProceedings of the National Academy of Sciences of the United States of America. 2014;111(24):8764-9
Accuracy tests of radiation schemes used in hot Jupiter global circulation models1402.0814v2 · David Sk\aalid Amundsen, Isabelle Baraffe, Pascal Tremblin et al.2014 · 182 citationsarXivon Valency
The UM, a fully--compressible, non--hydrostatic, deep atmosphere GCM, applied to hot Jupiters1311.2083v1 · N. J. Mayne, I. Baraffe, David M. Acreman et al.2013 · 0 citationsarXiv
Using the UM dynamical cores to reproduce idealised 3D flows1310.6041v1 · N. J. Mayne, I. Baraffe, David M. Acreman et al.2013 · 75 citationsarXiv
Transition from static to kinetic friction: insights from a 2D model.21902397 · Trømborg, J, Scheibert, J, Amundsen, D S et al.2012 · 89 citationsPhysical review letters. 2011;107(7):074301
Career total: 63 works. 28 are in this corpus.
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