9–12 Sept 2024
University Oxford
Europe/London timezone

Emission spectroscopy of ablative heat shield shock layers for earth entry in the T6 free piston driven shock tube

12 Sept 2024, 16:40
25m
Oxford e-Research Centre (University Oxford)

Oxford e-Research Centre

University Oxford

7 Keble Rd, Oxford OX1 3QG United Kingdom
High speed facilities, flight testing and propulsion High speed facilities, flight testing and propulsion

Speaker

Mr Aaron Kennedy (University of Oxford)

Description

See attached

Summary

This paper shows the results of an emission spectroscopy test campaign completed in Oxford’s T6 free piston driven Shock tube. Ablative thermal protection systems have proven to be a common option utilised on spacecraft returning to earth in the brief time mankind has been conducting space missions. The pyrolysis gasses produced by ablative heat shields while undergoing heating from an earth entry trajectory changes the composition of the gas species in the shock layer surrounding the craft. The presence of new molecules augment the thermochemical relaxation processes and in turn augment the heat flux acting on the vehicles surface. Emission spectra has been captured for two analogous pyrolysis/atmospheric air mixtures at varying shock speeds and initial fill pressures. This aimed to analyse the spectra at a non exhaustive list of flight velocities and altitudes. The spectra along with the radiance profile behind the shock are presented for each condition for both UV/vis and visible/IR parts of the spectrum.

Primary author

Mr Aaron Kennedy (University of Oxford)

Co-authors

Mr Alex Glenn (University of Oxford) Matthew Mcgilvray (University of Oxford)

Presentation materials