Start Date

29-2-2012 8:40 AM

Description

The great majority of modern space vehicles designed for planetary exploration use ablative materials to protect the payload against the high heating environment experienced during re-entry. In order to properly model and predict the aerothermal environment of the vehicle, it is imperative to account for the gases produced by ablation processes. In the case of charring ablators, where an inner resin is pyrolyzed at a relatively low temperature, the composition of the gas expelled into the boundary layer is complex and may lead to thermal chemical reactions that cannot be captured with simple flow chemistry models. In order to obtain better predictions, an appropriate gas flow chemistry model needs to be included in the CFD calculations. The effects of allowing such gaseous species to form in the flow field have notable repercussions on the amount of heat fluxes to the surfaces.

Notes

The presentation slides are available by clicking the Download button on the right.

The complete abstract and figures are available as the additional file listed below.

2012_Martin_modeling.pdf (159 kB)
Abstract and figures

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Feb 29th, 8:40 AM

Modeling of Heat Transfer Attenuation by Ablative Gases during the Stardust Re-Entry

The great majority of modern space vehicles designed for planetary exploration use ablative materials to protect the payload against the high heating environment experienced during re-entry. In order to properly model and predict the aerothermal environment of the vehicle, it is imperative to account for the gases produced by ablation processes. In the case of charring ablators, where an inner resin is pyrolyzed at a relatively low temperature, the composition of the gas expelled into the boundary layer is complex and may lead to thermal chemical reactions that cannot be captured with simple flow chemistry models. In order to obtain better predictions, an appropriate gas flow chemistry model needs to be included in the CFD calculations. The effects of allowing such gaseous species to form in the flow field have notable repercussions on the amount of heat fluxes to the surfaces.