Hierarchical modeling of solar system planets with Isca
dc.contributor.author | Thomson, SI | |
dc.contributor.author | Vallis, GK | |
dc.date.accessioned | 2020-04-01T10:56:37Z | |
dc.date.issued | 2019-12-12 | |
dc.description.abstract | We describe the use of Isca for the hierarchical modeling of Solar System planets, with particular attention paid to Earth, Mars, and Jupiter. Isca is a modeling framework for the construction and use of models of planetary atmospheres at varying degrees of complexity, from featureless model planets with an atmosphere forced by a thermal relaxation back to a specified temperature, through aquaplanets with no continents (or no ocean) with a simple radiation scheme, to near-comprehensive models with a multi-band radiation scheme, a convection scheme, and configurable continents and topography By a judicious choice of parameters and parameterization schemes, the model may be configured for fairly arbitrary planets, with stellar radiation input determined by astronomical parameters, taking into account the planet's obliquity and eccentricity In this paper, we describe the construction and use of models at varying levels of complexity for Earth, Mars and Jupiter using the primitive equations and/or the shallow water equations. | en_GB |
dc.description.sponsorship | Leverhulme Trust | en_GB |
dc.identifier.citation | Vol. 10 (12), article 803 | en_GB |
dc.identifier.doi | 10.3390/ATMOS10120803 | |
dc.identifier.uri | http://hdl.handle.net/10871/120490 | |
dc.language.iso | en | en_GB |
dc.publisher | MDPI | en_GB |
dc.relation.url | https://github.com/ExeClim/Isca | en_GB |
dc.rights | © 2019 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). | en_GB |
dc.subject | planetary atmospheres | en_GB |
dc.subject | general circulation models | en_GB |
dc.subject | climate models | en_GB |
dc.subject | model hierarchy | en_GB |
dc.title | Hierarchical modeling of solar system planets with Isca | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2020-04-01T10:56:37Z | |
dc.description | This is the final version. Available from MDPI via the DOI in this record. | en_GB |
dc.description | All of the code necessary to run Isca, including the experiments described in this paper, are available on GitHub at https://github.com/ExeClim/Isca. | en_GB |
dc.identifier.journal | Atmosphere | en_GB |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | en_GB |
dcterms.dateAccepted | 2019-12-02 | |
rioxxterms.version | VoR | en_GB |
rioxxterms.licenseref.startdate | 2019-12-02 | |
rioxxterms.type | Journal Article/Review | en_GB |
refterms.dateFCD | 2020-04-01T10:51:16Z | |
refterms.versionFCD | VoR | |
refterms.dateFOA | 2020-04-01T10:56:41Z | |
refterms.panel | B | en_GB |
refterms.depositException | publishedGoldOA |
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Except where otherwise noted, this item's licence is described as © 2019 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).