Show simple item record

dc.contributorSoria Guerrero, Manel
dc.contributorGarcía Melendo, Enrique José
dc.contributor.authorMoya Acosta, Leonardo Andrés
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2020-10-23T09:07:51Z
dc.date.available2020-10-23T09:07:51Z
dc.date.issued2020-07
dc.identifier.urihttp://hdl.handle.net/2117/330699
dc.description.abstractThe current software for planetary atmosphere simulations, at the moment of writing this thesis, is limited to a Shallow-Water mono-layer model. This document presents the multi-layer model in isopycnical coordinates with topography implementation, as well as its numerical integration in the new SA3 code environment developed by the research group TUAREG. A series of benchmark cases is provided for verification purposes of the model. Then, a set of study cases on storms in Saturn and the Great Red Spot in Jupiter are described with the intention understanding planetary atmospheres phenomenology. Additionally, given the capabilities of the software, a research study of orographic waves generated by the Amsterdam Island is displayed.
dc.language.isoeng
dc.publisherUniversitat Politècnica de Catalunya
dc.rightsReconeixement-NoComercial-Compartir Igual 3.0 Espanya
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshPlanets--Atmospheres
dc.subject.lcshComputer simulation
dc.titleHigh performance computing simulation of planetary atmospheres
dc.typeMaster thesis
dc.subject.lemacPlanetes -- Atmòsferes
dc.subject.lemacSimulacio per ordinador
dc.identifier.slugPRISMA-153430
dc.rights.accessOpen Access
dc.date.updated2020-08-26T18:52:48Z
dc.audience.educationlevelMàster
dc.audience.mediatorEscola Superior d'Enginyeries Industrial, Aeroespacial i Audiovisual de Terrassa
dc.audience.degreeMÀSTER UNIVERSITARI EN ENGINYERIA AERONÀUTICA (Pla 2014)


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record