Zobrazeno 1 - 10
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pro vyhledávání: '"Skinner, J. A."'
Autor:
Skinner, J. W., Cho, J. Y-K.
We report on the critical influence of small-scale flow structures (e.g., fronts, vortices, and waves) that immediately arise in hot-exoplanet atmosphere simulations initialized with a resting state. A hot, 1:1 spin-orbit synchronized Jupiter is used
Externí odkaz:
http://arxiv.org/abs/2406.00526
Autor:
Alexandre Dittrich
Publikováno v:
Psicologia: Reflexão e Crítica, Vol 21, Iss 2, Pp 252-260 (2008)
Um dos aspectos mais interessantes e polêmicos da obra de B. F. Skinner é sua interpretação sobre a evolução das culturas. De acordo com o autor, as conseqüências de práticas culturais retroagem sobre as culturas, no sentido de aumentar ou d
Externí odkaz:
https://doaj.org/article/2e5209c85b9b4465ad32e3580be9d6d0
Autor:
Alexandre Dittrich
Publikováno v:
Psicologia: Reflexão e Crítica, Vol 21, Iss 2, Pp 252-260 (2008)
One of the most interesting and polemic features of B. F. Skinner's work is his interpretation about cultural evolution. According to that author, the consequences of cultural practices have a retroactive effect over the cultures, increasing or decre
Externí odkaz:
https://doaj.org/article/c4e0eb7d3d3747dba07745113100d92f
Publikováno v:
Physical Review Letters, 131, 231201, 2023
Most current models of hot-exoplanet atmospheres assume shallow heating, a strong day-night differential heating near the top of the atmosphere. Here we investigate the effects of energy deposition at differing depths in a model tidally locked gas-gi
Externí odkaz:
http://arxiv.org/abs/2212.05114
Autor:
Skinner, J. W., Cho, J. Y-K.
We investigate modons on tidally synchronised extrasolar planets. Modons are highly dynamic, coherent flow structures composed of a pair of storms with opposite signs of vorticity. They are important because they divert flows on the large-scale; and,
Externí odkaz:
http://arxiv.org/abs/2109.06568
Observations of hot-Jupiter atmospheres show large variations in the location of the hot spot and the amplitude of spectral features. Atmospheric flow simulations using the commonly-employed forcing and initialization have generally produced a large,
Externí odkaz:
http://arxiv.org/abs/2105.12759
Akademický článek
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Autor:
Cho, J. Y-K., Thrastarson, H. Th., Koskinen, T. T., Read, P. L., Tobias, S. M., Moon, W., Skinner, J. W.
We review the recent progress in understanding the jet structures on exoplanets as well as on and inside the Sun. The emphasis is on the more robust aspects of observation and numerical modeling that relate directly to jets. For the exoplanets, the p
Externí odkaz:
http://arxiv.org/abs/2010.09878
Autor:
Skinner, J. W., Cho, J. Y-K.
We perform an extensive study of numerical convergence for hot-Jupiter atmospheric flow solutions in simulations employing a setup commonly-used in extrasolar planet studies, a resting state thermally forced to a prescribed temperature distribution o
Externí odkaz:
http://arxiv.org/abs/2010.09695
Autor:
Philip A. Harland
Publikováno v:
Mnemosyne. 68:682-684
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7d9eb6649d5c646005306812dd83af65
https://doi.org/10.1163/1568525x-12341888
https://doi.org/10.1163/1568525x-12341888