Aerodynamics of a wing section along an entry path in Mars atmosphere

被引:4
|
作者
Zuppardri, Gennaro [1 ]
Mongelluzzo, Giuseppe [1 ,2 ]
机构
[1] Univ Naples Federico II, Dept Ind Engn, Piazzale Tecchio 80, I-80125 Naples, Italy
[2] INAF Astron Observ Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy
来源
关键词
wing section Aerodynamics; hypersonic flow; direct simulation Monte Carlo method; wing-flap deflection; shock wave-shock wave interaction;
D O I
10.12989/aas.2021.8.1.053
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The increasing interest in the exploration of Mars stimulated the authors to study aerodynamic problems linked to space vehicles. The aim of this paper is to evaluate the aerodynamic effects of a flapped wing in collaborating with parachutes and retro-rockets to reduce velocity and with thrusters to control the spacecraft attitude. 3-D computations on a preliminary configuration of a blunt-cylinder, provided with flapped fins, quantified the beneficial influence of the fins. The present paper is focused on Aerodynamics of a wing section (NACA-0010) provided with a trailing edge flap. The influence of the flap deflection was evaluated by the increments of aerodynamic force and leading edge pitching moment coefficients with respect to the coefficients in clean configuration. The study was carried out by means of two Direct Simulation Monte Carlo (DSMC) codes (DS2V/3V solving 2-D/3-D flow fields, respectively). A DSMC code is indispensable to simulate complex flow fields on a wing generated by Shock Wave-Shock Wave Interaction (SWSWI) due to the flap deflection. The flap angle has to be a compromise between the aerodynamic effectiveness and the increases of aerodynamic load and heat flux on the wing section lower surface.
引用
收藏
页码:53 / 67
页数:15
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