Stability analysis of two-dimensional flat solar trackers using aerodynamic derivatives at different heights above ground

Cárdenas Rondón, Juan Andrés ORCID: https://orcid.org/0000-0003-2962-1620, Ogueta Gutiérrez, Mikel ORCID: https://orcid.org/0000-0001-9183-450X, Franchini Longhi, Sebastian Nicolas ORCID: https://orcid.org/0000-0002-1476-9174 and Manzanares Bercial, Raúl ORCID: https://orcid.org/0000-0001-8987-1694 (2023). Stability analysis of two-dimensional flat solar trackers using aerodynamic derivatives at different heights above ground. "Journal of Wind Engineering and Industrial Aerodynamics", v. 243 ; p. 105606. ISSN 01676105. https://doi.org/10.1016/j.jweia.2023.105606.

Descripción

Título: Stability analysis of two-dimensional flat solar trackers using aerodynamic derivatives at different heights above ground
Autor/es:
Tipo de Documento: Artículo
Título de Revista/Publicación: Journal of Wind Engineering and Industrial Aerodynamics
Fecha: 1 Diciembre 2023
ISSN: 01676105
Volumen: 243
Materias:
ODS:
Palabras Clave Informales: Aerodynamic instability; Identification; model; Solar tracker; wind tunnel; Aerodynamic derivatives; AERODYNAMIC INSTABILITY; FLUTTER DERIVATIVES; solar tracker; Wind tunnel
Escuela: E.T.S. de Ingeniería Aeronáutica y del Espacio (UPM)
Departamento: Aeronaves y Vehículos Espaciales
Licencias Creative Commons: Reconocimiento - No comercial

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Resumen

In this paper the aerodynamic stability of a flat-plate solar tracker under two-dimensional conditions is studied for different conditions of incident wind speed, U∞, nominal angle of attack, αn∈−40∘,40∘, and shaft height - chord ratio H/B=0.3,0.4,0.5,0.6,1and2. The stability is studied through the analysis of the aerodynamic derivatives A2∗ and A3∗ whose behaviours as a function of U∞ are presented for the H/B range studied. Two methods of obtaining the derivatives (one in the time domain and the other one in the frequency domain) are presented. A method for calculating the effective damping coefficient of the solar tracker, ξeff, as a function of the incident wind speed, U∞, is presented. This method can be used for any solar tracker structural characteristics (Jmech, Cmech and Kmech). With this method, the critical speed, Ucrit, can be determined by imposing the condition ξeff=0. The method was validated experimentally using the results of two different experimental set-ups.

Proyectos asociados

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Código
Acrónimo
Responsable
Título
Gobierno de España
TED2021-130541B-C21
Sin especificar
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Gobierno de España
PID2022-137630OB-C21
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Más información

ID de Registro: 94140
Identificador DC: https://oa.upm.es/94140/
Identificador OAI: oai:oa.upm.es:94140
URL Portal Científico: https://portalcientifico.upm.es/es/ipublic/item/10113942
Identificador DOI: 10.1016/j.jweia.2023.105606
URL Oficial: https://www.sciencedirect.com/science/article/pii/...
Depositado por: iMarina Portal Científico
Depositado el: 19 Feb 2026 11:39
Ultima Modificación: 19 Feb 2026 11:39