ExoMars Flush Air Data System: Entry Simulation and Atmospheric Reconstruction Method

被引:7
作者
Van Hove, Bart [1 ]
Karatekin, Ozgur [1 ]
Schleutker, Thorn [2 ]
Guelhan, Ali [3 ]
机构
[1] Royal Observ Belgium, Dept Reference Syst & Planetol, B-1180 Brussels, Belgium
[2] German Aerosp Ctr, DLR, Superson & Hyperson Technol Dept, Inst Aerodynam & Flow Technol, D-51147 Cologne, Germany
[3] German Aerosp Ctr, DLR, Dept & Superson & Hyperson Technol Dept, Inst Aerodynam & Flow Technol, D-51147 Cologne, Germany
基金
欧盟地平线“2020”;
关键词
SCIENCE LABORATORY ENTRY; MARS PHOENIX ENTRY; DESCENT; AERODYNAMICS;
D O I
10.2514/1.A34187
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Flight data recorded during atmospheric entry with forebody pressure instrumentation, referred to as a flush air data system (FADS), provide valuable measurements for the reconstruction of the trajectory and in situ atmospheric conditions. We present a method to reconstruct the angle of attack; sideslip angle; and atmospheric density, pressure, and temperature in support of the postflight analysis for the ExoMars Entry, Descent, and Landing Demonstrator Module (EDM), named Schiaparelli. Numerical predictions of the forebody surface pressure distribution, required as input to the FADS reconstruction, were developed in a companion paper. Here, we demonstrate the FADS method in a hypersonic wind tunnel at Mach 5 to 7 and study theoretical FADS reconstruction performance along a simulated along a simulated entry trajectory. The main error sources identified are unobserved winds and measurement bias errors; the latter are exacerbated by the limited number of pressure ports on the EDM.
引用
收藏
页码:1205 / 1220
页数:16
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