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Reduced Chemical Kinetic Model for Titan Entries

Published:2011 Issue: Volume:2011 Page:1-8
ISSN:1687-806X
Container-title:International Journal of Chemical Engineering
language:en
Short-container-title:International Journal of Chemical Engineering

Author:

Savajano Romain¹,Sobbia Raffaello¹,Gaffuri Michele¹²,Leyland Pénélope¹

Affiliation:

1. Ecole Polytechnique Fédérale de Lausanne, Interdisciplinary Aerodynamics Group, Station 9, 1015 Lausanne, Switzerland

2. Deutsches Zentrum für Luft- und Raumfahrt (DLR), Lilienthalplatz 7, 38108 Braunschweig, Germany

Abstract

A reduced chemical kinetic model for Titan's atmosphere has been developed. This new model with 18 species and 28 reactions includes the mainfeatures of a more complete scheme, respecting the radiative fluxes. It has been verified against three key elements: a sensitivity analysis, the equilibrium chemical composition using shock tube simulations in CHEMKIN, and the results of computational fluid dynamics (CFDs) simulations.

Funder

ESA-NPI Program

Publisher

Hindawi Limited

Subject

General Chemical Engineering

Link

http://downloads.hindawi.com/journals/ijce/2011/970247.pdf

Reference19 articles.

1. Titan atmospheric composition by hypervelocity shock-layer analysis

2. Numerical Computation of Radiative Heating Environment for Huygens Probe Entry Flight

3. N2-CH4-Ar Chemical Kinetic Model for Simulations of Atmospheric Entry to Titan

4. Modeling and Experimental Assessment of CN Radiation Behind a Strong Shock Wave

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1. Non-equilibrium and anisotropy in Titan atmosphere entry;Advances in Space Research;2024-07

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3. Aerodynamic Analysis of an Entry Capsule at Titan in Transition Regime;Journal of Spacecraft and Rockets;2023-03

4. On the Formation and Accumulation of Solid Carbon Particles in High-Enthalpy Flows Mimicking Re-Entry in the Titan Atmosphere;Fluids;2020-06-12

5. Combining particle-in-cell and direct simulation Monte Carlo for the simulation of reactive plasma flows;Physics of Fluids;2019-07

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