Repositori institucional URV
| Autor/es de la URV: | Dubert, Diana Cristina / Gavaldà Martínez, Josefa / Masons Bosch, Jaime / Ruiz Plazas, Xavier / Simón Olmos, María José |
| Autor según el artículo: | Dubert, D; Simón, MJ; Massons, J; Ruiz, X; Gavaldà, J |
| Direcció de correo del autor: | xavier.ruiz@urv.cat dianacristina.dubert@urv.cat jaume.masons@urv.cat fina.gavalda@urv.cat mariajose.simon@urv.cat |
| Identificador del autor: | 0000-0002-7308-5872 0000-0003-4325-6084 0000-0001-7881-4192 0000-0002-4885-5935 |
| Año de publicación de la revista: | 2024 |
| Tipo de publicación: | Journal Publications |
| Referencia de l'ítem segons les normes APA: | Dubert, D; Simón, MJ; Massons, J; Ruiz, X; Gavaldà, J (2024). Numerical analysis of n-octadecane melting process in a rectangular cell under reboosting maneuver conditions. Acta Astronautica, 215(), 455-463. DOI: 10.1016/j.actaastro.2023.12.020 |
| Referencia al articulo segun fuente origial: | Acta Astronautica. 215 455-463 |
| Resumen: | The improvement of heat management based on Phase Change Materials (PCMs) is of increasing importance in space environments. In this context, a future ESA project called Effect of Marangoni Convection on heat transfer in Phase Change Materials (MarPCM) will evaluate the degree of improvement in heat transport using thermocapillarity as convective activator of the liquid phase generated during the melting. Since this type of project needs to be performed onboard International Space Station, ISS, it is of outmost importance to know if the accelerometric environment of the Station could affect the experiment results.To do so, various 2D simulations of the solid-liquid phase change were carried out using n-octadecane as PCM material, by considering a pre-selected acceleration signal coming from a real ISS reboosting maneuver (June 24, 2021). Different gravity scenarios have been considered by changing both the intensity and the orientation of the reboosting maneuver, parallel (x direction) and perpendicular (y direction) to the thermal gradients. The acceleration levels were enhanced up to 1000 times the intensity achieved during the real reboosting in order to predict the safety margins of the ISS experiment.The results showed alterations of the liquid-solid interface, during the melting process in the high g-level scenarios considered. In these cases, the oscillatory flow pattern became more complex detecting sudden changes in the main frequency which were maintained approximately 1000 s after the reboosting ended. Nevertheless, applying real boosting maneuver no significant influence in the melting process was detected. |
| DOI del artículo: | 10.1016/j.actaastro.2023.12.020 |
| Enlace a la fuente original: | https://www.sciencedirect.com/science/article/pii/S0094576523006501?via%3Dihub |
| Versión del articulo depositado: | info:eu-repo/semantics/publishedVersion |
| Acceso a la licencia de uso: | https://creativecommons.org/licenses/by/3.0/es/ |
| Departamento: | Química Física i Inorgànica Enginyeria Mecànica |
| URL Documento de licencia: | https://repositori.urv.cat/ca/proteccio-de-dades/ |
| Áreas temáticas: | Interdisciplinar Geociências Engineering, aerospace Engenharias iv Engenharias iii Engenharias ii Ciência da computação Astronomia / física Aerospace engineering & technology Aerospace engineering |
| Palabras clave: | Thermocapillary convection (marangoni effect) Phase-change materials Phase change materials Openfoam software Iss vibrational environment Environment Energy-storage Accelerations |
| Entidad: | Universitat Rovira i Virgili |
| Fecha de alta del registro: | 2024-08-03 |
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