Title:
Ablation of Pica-Like Material: Surface or Volume Phenomenon?

dc.contributor.author Lachaud, Jean en_US
dc.contributor.author Mansour, Nagi Nicolas en_US
dc.contributor.corporatename Ames Research Center en_US
dc.contributor.corporatename United States. National Aeronautics and Space Administration
dc.date.accessioned 2009-01-20T19:50:59Z
dc.date.available 2009-01-20T19:50:59Z
dc.date.issued 2008-06-26
dc.description This presentation was part of the session : Current Planetary Probe Science and Technology en_US
dc.description Sixth International Planetary Probe Workshop en_US
dc.description.abstract The ablation of the char layer in ablative material is usually described in term of recession velocity of the overall surface. This description is valid for dense materials. However, the recession of the average surface in porous materials may not recede uniformly, but the individual fibers may progressively vanish. In the second regime, ablation is no longer a surface phenomenon, but is volumetric. Seen from a surface point of view, three important consequences follow this volume ablation regime: (1) the effective reactivity of the material is significantly increased, (2) the material weakens in volume and is subject to strong mechanical erosion (spallation), and (3) the ablation enthalpy distributed in volume modifies the thermal response of the material. In this regime, surface ablation models should be replaced by volume ablation models for a more accurate description of the outer layer of the material. In the presentation, a first attempt to couple volume ablation with pyrolysis is done using a multiscale approach. In an effort to derive phenomenological models for the volume ablation regime, three-dimensional (3D) simulations of isothermal ablation in air of a low-density material made of carbon fibers distributed randomly are performed. A parametric study shows that ablation is either a surface or a volume phenomenon depending on the value of Thiele number (reaction/diffusion competition inside the porous media), when advection due to pyrolysis and thermal gradients are neglected. A macroscopic model for volume ablation is derived analytically using homogenization (averaging). The model is a set of partial differential equations, similar to traditional pyrolysis models. Simulations of coupled pyrolysis and volume ablation are presented. The possible spallation of PICA due to volume ablation during Stardust re-entry is discussed under the light of this model. en_US
dc.description.sponsorship NASA Ames Research Center en_US
dc.identifier.uri http://hdl.handle.net/1853/26333
dc.publisher Georgia Institute of Technology en_US
dc.relation.ispartofseries IPPW08. Current Planetary Probe Science and Technology en_US
dc.subject Ablation en_US
dc.subject Pyrolysis en_US
dc.subject Spallation en_US
dc.subject Stardust en_US
dc.title Ablation of Pica-Like Material: Surface or Volume Phenomenon? en_US
dc.type Text
dc.type.genre Proceedings
dspace.entity.type Publication
local.contributor.corporatename Daniel Guggenheim School of Aerospace Engineering
local.contributor.corporatename College of Engineering
local.relation.ispartofseries International Planetary Probe Workshop (IPPW)
relation.isOrgUnitOfPublication a348b767-ea7e-4789-af1f-1f1d5925fb65
relation.isOrgUnitOfPublication 7c022d60-21d5-497c-b552-95e489a06569
relation.isSeriesOfPublication 6369d36f-9ab2-422f-a97e-4844b98f173b
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