Team building at institute level
Contact - Personnal web page
Supervisor(s): Philippe Chatelain
This project aims to a detailed modelling of a meteoroid entry into planet Earth. The state-of-the-art models to simulate the meteoroid demise rely simplified assumptions where flow/meteoroid ablation interaction are often neglected. For instances the multiphase problem due to the melting of the meteoroid is not considered.
The approach considered in this project considers the developing of models containing melting/evaporation information which can be included in CFD solvers. Hereafter we could to simulate a meteoroid entry where radiation is also included and compared with observations done by the scientific community.
The preliminary results shows that the molten layer removal due to shear forces is the major source of the ablation process for low altitudes conditions. Also with the increase of the body radius the radiation becomes dominant as a heat source.
IMMC main research direction(s):
Research group(s): TFL
See complete list of publications
1. Dias, Bruno; Bariselli, Federico; Turchi, Alessandro; Frezzotti, Aldo; Chatelain, Philippe; Magin, Thierry. Development of a melting model for meteors. In: AIP Conference Proceedings. Vol. 1786, no.1, p. 160004 (2016). doi:10.1063/1.4967661. http://hdl.handle.net/2078.1/182548