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Characterization of carbon-fiber reinforced ultra-high-temperature ceramic matrix composites in arc-jet environment

Contributo in Atti di convegno
Data di Pubblicazione:
2018
Abstract:
In the framework of the Horizon 2020 project CHARME, an experimental campaign has been carried out to characterize a new class of Ultra-High-Temperature Ceramic Matrix Composites for near-zero ablation Aerospace Thermal Protection Systems. Small sized specimens, with ZrB2-based matrix and different carbon fiber architectures, were exposed to a supersonic flow of simulated air generated by an arc-jet wind tunnel, achieving specific total enthalpies up to 20 MJ/kg, in an aero-thermo-chemical environment representative of atmospheric re-entry. Ablation rates were estimated by means of mass and thickness measurements before and after testing, demonstrating a good performance of the analyzed samples, although with some mechanical resistance issues. Surface temperatures were monitored by means of infrared pyrometers and a thermo-camera, and during most of the tests a spontaneous temperature jump was observed, with temperatures that reached values over 2800 K at the steady state. Computational Fluid Dynamics simulations allowed for the rebuilding of the thermo-fluid-dynamic and chemical flow field. Moreover, it was possible to propose a correlation of the temperature jump with an increased catalytic activity and a dramatic reduction of the thermal conductivity of the oxide layers forming on the exposed part of the sample, which anyway had a key role in preserving the unoxidized bulk materials at reasonable temperatures.
Tipologia CRIS:
04.01 Contributo in Atti di convegno
Keywords:
Arc-jet wind tunnel testing; Computational Fluid Dynamic simulation; Near-zero ablation; Oxidation; Temperature Jump; Ultra-High-Temperature Ceramic Matrix Composites
Elenco autori:
Sciti, Diletta; Silvestroni, Laura; Zoli, Luca
Autori di Ateneo:
SCITI DILETTA
SILVESTRONI LAURA
ZOLI LUCA
Link alla scheda completa:
https://iris.cnr.it/handle/20.500.14243/443827
Pubblicato in:
PROCEEDINGS OF THE INTERNATIONAL ASTRONAUTICAL CONGRESS
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http://www.scopus.com/record/display.url?eid=2-s2.0-85065323932&origin=inward
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