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dc.contributorGarcía Melendo, Enrique José
dc.contributorSoria Guerrero, Manel
dc.contributor.authorBiosca Llorente, Joel
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2023-07-07T10:38:46Z
dc.date.issued2023-05-19
dc.identifier.urihttp://hdl.handle.net/2117/390468
dc.description.abstractThis project consists of the programming, following an already established method; and execution of a simplified numerical model based on the Navier-Stokes equations, the Shallow Water 2D model, to simulate large-scale planetary atmospheric phenomena; concretely Jupiter Great Red Spot (without viscosity but in the presence of rotation and in elipsoidal coordinates). The phases are: understanding the Navier-Stokes equations and the simplifications that lead to the Shallow Water model, programming each point of this model in a specific order, as well as verifying each step, this process is called step-by-step method; running concrete simulations and comparing the final results with real phenomena. Since this thesis belongs to a group of works in the same field carried out in the past, it can be consulted in the future by other students. For this reason, it is written in a clear way, and its reading order is as linear as possible. Moreover, during the constitution of the model, those aspects that could differ from the generalised paradigm, established over several theses, are rigorously explained, as well as are explicited concepts that are not usually mentioned but are clarifying. The results obtained are generally adequate, compared with different sources, except for some simulations with Coriolis in Cartesian that perhaps dissipate too much. But in later more complex simulations where the accuracy has been increased, results have been obtained in line with certain sources and comparable to the real Jupiter Great Red Spot. The rest of the objectives have also been met satisfactorily, improving personally programming skills and understanding of fluid mechanics and its numerical implementation.
dc.language.isoeng
dc.publisherUniversitat Politècnica de Catalunya
dc.subjectÀrees temàtiques de la UPC::Física
dc.subjectÀrees temàtiques de la UPC::Matemàtiques i estadística::Equacions diferencials i integrals
dc.subject.lcshAtmosphere -- Computer simulation
dc.subject.otherShallow Water model
dc.subject.otherMecànica de fluids
dc.subject.otherMètodes numèrics
dc.subject.otherProgramació
dc.titleImplementation of a 2D model of a planetary atmosphere
dc.typeBachelor thesis
dc.subject.lemacAtmòsfera -- Simulació per ordinador
dc.identifier.slugPRISMA-173600
dc.rights.accessRestricted access - author's decision
dc.date.lift10000-01-01
dc.date.updated2023-06-07T18:33:59Z
dc.audience.educationlevelGrau
dc.audience.mediatorEscola Superior d'Enginyeries Industrial, Aeroespacial i Audiovisual de Terrassa
dc.audience.degreeGRAU EN ENGINYERIA EN TECNOLOGIES AEROESPACIALS (Pla 2010)


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