CONFERENCE PAPER - Investigation of GSI and Modeling of Catalycity for TPM testing in PWT

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63rd International Astronautical Congress, Naples, Italy. Copyright Š2012 by the International Astronautical Federation. All rights reserved.

IAC-12-C2.8.8 INVESTIGATION OF GAS-SURFACE INTERACTIONS AND MODELLING OF THE REFERENCE CATALYCITY FOR THERMAL PROTECTION MATERIAL TESTING IN PLASMA WIND TUNNELS Guerric de Crombrugghe* von Karman Institute, Belgium, g.crombrugg@gmail.com Olivier Chazot von Karman Institute, Belgium, chazot@vki.ac.be Atmospheric re-entry is integral to further developments in space exploration, whether it concerns the safe return of astronauts or payload to Earth or the landing of robots on Mars, Venus, and even Titan. Despite the important heritage acquired since the beginning of the space age, it remains a complicated field of study, especially when it comes to super-orbital re-entry. The understanding of the chemistry processes taking place in the boundary layer is among the areas of improvement for the design of re-entry vehicles. One of the main parameters currently used for the sizing of thermal protection systems (TPS) is the catalycity of the thermal protection material (TPM), usually defined as the ratio between the number of atoms that recombine on the surface and the number of atoms that impact it. As recombination is an exothermic process, high catalycity is undesirable as it increases the heat flux that the thermal protection system has to withstand. Catalycity is experimentally determined in plasma wind tunnels, based on the comparison with a material of known catalycity. That reference is often a copper sample, assumed to be of high catalycity. However, it was demonstrated in previous studies that this assumption is not always correct, resulting in an over-estimation of TPM catalycity and over-sizing of TPS. Space missions with stringent mass budget are therefore penalized with heavier heat shield and reduced payload mass. A new model for the reference catalycity is thus necessary, especially for super-orbital entries. This paper presents a qualitative analysis of the relative influence of all the test parameters involved in experimental determination of gas-surface interactions (GSI) phenomena for wall catalysis. The analysis is based on experimental results obtained in the von Karman Institute’s Plasmatron, and numerical rebuilding of the boundary layer with in-house software. It appears that the wall recombination coefficient depends on the material properties as well as the environment conditions through a diffusion-reaction process. I.

INTRODUCTION

Since the very beginning of the space age, atmospheric re-entry has been considered as an important area of study. It is a key to further developments in space exploration, whether it concerns the safe return of astronauts and payloads to Earth or the landing of robots on Mars, Venus, and even Titan. One of the main areas of improvement for the design of reentry vehicles is the understanding of the gas-surface interactions (GSI) processes in flight conditions. Within that scope, this paper presents experimental research that was conducted on the driving processes of GSI over a cold copper wall in order to provide a foundation for an accurate model of wall catalycity. Those investigations are based on experimentations performed at the von Karman Institute (VKI) in the Plasmatron, an Inductive Coupled Plasma (ICP) wind tunnel, and numerical rebuilding of the boundary layer with in-house software. The issue of catalycity modelling and its importance in the frame of re-entry technologies is first presented together with a definition of the investigated GSI parameters. The facilities and methods for catalycity

IAC-12-C2.8.8

and heat flux measurements are then described, as well as the experimental campaigns conducted. The GSI are then analyzed in details through the qualitative evolution of GSI parameters depending on the test parameters. Finally, recommendations are given for a more developed model of catalycity. The results presented in this paper are the extension of a research project available in (de Crombrugghe 2012). II.

CATALYCITY MODELLING

High-temperature gas dynamics When a vehicle flies in hypersonic regime, a strong bow shock appears in front of its nose. Across that shock, a considerable part of the flow's kinetic energy will be transformed in thermal energy. The shock-layer temperature achieved is considerable: from 8,000 K for an orbital re-entry up to 11,000 K for a lunar return, and even higher for super-orbital re-entry. At such temperatures, chemical effects have to be taken into account. For air at a pressure of 1 atm, vibrational excitation begins at 800 K, O2 begins to dissociate at 2,500 K and is fully dissociated for 4,000 K, point for

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