HEAL DSpace

Προσομοίωση ροής γύρω από συστοιχία φωτοβολταϊκών συλλεκτών

Αποθετήριο DSpace/Manakin

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dc.contributor.author Τζέκος, Παναγιώτης el
dc.contributor.author Tzekos, Panagiotis en
dc.date.accessioned 2024-07-11T06:27:27Z
dc.date.available 2024-07-11T06:27:27Z
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/59847
dc.identifier.uri http://dx.doi.org/10.26240/heal.ntua.27543
dc.description Εθνικό Μετσόβιο Πολυτεχνείο--Μεταπτυχιακή Εργασία. Διεπιστημονικό-Διατμηματικό Πρόγραμμα Μεταπτυχιακών Σπουδών (Δ.Π.Μ.Σ.) “Υπολογιστική Μηχανική” el
dc.rights Default License
dc.subject Solar panels en
dc.subject Array en
dc.subject Ground mounted en
dc.subject Wind load en
dc.subject RANS en
dc.subject k-ε RNG en
dc.subject k-ω SST en
dc.title Προσομοίωση ροής γύρω από συστοιχία φωτοβολταϊκών συλλεκτών el
heal.type masterThesis
heal.classification Computational Fluid Dynamics en
heal.language el
heal.access free
heal.recordProvider ntua el
heal.publicationDate 2024-03-27
heal.abstract Photovoltaic arrays are primarily located in large open fields and often exposed to high wind speeds which result in the development of a complex flow field around them. These conditions cause significant aerodynamic loads which are exerted on the panels. Aerodynamics loads on, and wind flow field around, an array of ten ground mounted solar panels that are placed in an open field, are investigated using a steady state Reynolds-Averaged Navier–Stokes (RANS) approach. A full scale two-dimensional (2D) solver is employed with the Shear Stress Transport (SST) k–ω and Re-Normalisation Group k-ε (RNG) turbulence models. A grid independence study is conducted to ensure the accuracy of a single PV study case. Simulation results for the flow around a PV array are validated using wind tunnel experimental data. The effects of the Reynolds number on the calculation of pressure and force coefficients on the PVs are also investigated. The flow around the PV array is studied, considering the chosen geometric characteristics. A comparative analysis of the two turbulence models (k-ε RNG & k-ω SST) is carried out for both south and north wind directions. Parametric studies are conducted on the distance of the PVs from the ground and the distance between them, respectively. The force coefficient obtained from simulations is compared to that calculated by the Eurocode. The results show that all the trailing rows are in the wake of the leading row. For all the wind directions studied here, the first windward row experiences the maximum wind loads. As the distance from the ground decreases, the forces exerted on the panels also decrease. Also, the results showed that for the smallest distance ratio between the PVs, L/H=2.4, the force coefficient of the second PV exhibits a negative sign. Finally, the values of the force coefficient calculated by the Eurocode seem to overestimate the forces compared to those calculated from the simulations. en
heal.advisorName Bouris, Demetri en
heal.committeeMemberName Voutsinas, Spyridon en
heal.committeeMemberName Manolesos, Marinos en
heal.academicPublisher Εθνικό Μετσόβιο Πολυτεχνείο. Σχολή Χημικών Μηχανικών el
heal.academicPublisherID ntua
heal.numberOfPages 113 el
heal.fullTextAvailability false


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