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- W2341937013 abstract "Abstract for the 43rd AIAA Thermophysics Conference, New Orleans, LA, June 25-28, 2012 1 Experimental Validation of CO 2 Radiation Simulations Grant Palmer*, Brett Cruden * ERC Incorporated, Huntsville, AL 35805 I. Introduction pacecraft entering planetary atmospheres at high velocities will experience significant levels of radiative heating. In recent years, a number of studies have been performed to determine the vehicle and mission requirements that would enable the human exploration of Mars [1-4]. High-mass crewed Mars vehicles would be larger than previously-flown unmanned robotic spacecraft and would experience higher levels of radiative heating. Design of the vehicle heatshield and other components of the entry vehicle will require an accurate assessment of the radiative emission in the shock layer. The atmosphere of Mars is composed of primarily carbon dioxide (CO 2 ) and a small percentage of diatomic nitrogen. When the temperature in the shock layer is high, the primary radiators are CN and carbon monoxide (CO) [5]. At moderate temperatures of 3000-4000 K, the primary radiating species will be CO" @default.
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- W2341937013 date "2012-01-01" @default.
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- W2341937013 title "Experimental Validation of CO 2 Radiation Simulations" @default.
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