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首页> 外文期刊>Journal of Spacecraft and Rockets >Experimental Hypersonic Aerodynamic Characteristics of Mars Surveyor 2001 Precision Lander with Flap
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Experimental Hypersonic Aerodynamic Characteristics of Mars Surveyor 2001 Precision Lander with Flap

机译:带有襟翼的Mars Surveyor 2001精密着陆器的实验高超声速空气动力学特性

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Aerodynamic wind-tunnel screening tests were conducted on a 0.029-scale model of a proposed Mars Surveyor 2001 Precision Lander (70-deg half-angle spherically blunted cone with a conical afterbody). The primary experimental objective was to determine the effectiveness of a single flap to trim the vehicle at incidence during a lifting hypersonic planetary entry. The laminar force and moment data, presented in the form of coefficients, and shock patterns from schlieren photography were obtained in the facilities of the NASA Langley Aerothermodynamic Laboratory for postnormal shock Reynolds numbers (based on forebody diameter) ranging from 2.637 x 10~3 to 92.35 x 10~3, angles of attack ranging from 0 up to 23 deg at 0- and 2-deg sideslip, and normal-shock density ratios of 5 and 12. Based upon the proposed entry trajectory of the 2001 Lander, tests in the heavy gas CF4 simulate a Mach number of approximately 12 based upon a normal shock density ratio of 12 in flight at Mars. The results from this experimental study suggest that when the traditional means of providing aerodynamic trim for this class of planetary entry vehicle are not possible (e.g., offset e.g.), a single flap can provide similar aerodynamic performance. An assessment of blunt-body aerodynamic effects attributed to a real gas was obtained by synergistic testing in Mach 6 ideal air at a comparable Reynolds number. From an aerodynamic perspective, an appropriately sized flap was found to provide sufficient trim capability at the desired lift-to-drag ratio for precision landing. Inviscid hypersonic flow computations using an unstructured grid were made to provide an assessment of the viability of a flap to provide aerodynamic trim to the Lander. Subsequent Navier-Stokes computational predictions were found to be in very good agreement with experimental measurement.
机译:空气动力学风洞筛选测试是在拟议的Mars Surveyor 2001 Precision Lander(70度半角球形钝锥,带有锥形后座)的0.029比例模型上进行的。主要的实验目标是确定在提升高超音速行星进入过程中单个襟翼在入射时修剪车辆的有效性。以系数形式表示的层流力和力矩数据以及来自schlieren摄影的冲击波模式是在NASA Langley空气热力学实验室的设施中获得的,其正常冲击后雷诺数(基于前体直径)范围为2.637 x 10〜3到92.35 x 10〜3,迎角在0和2度侧滑时从0到23度不等,法向冲击密度比为5和12。根据2001年Lander的拟议进入轨迹,在重气体CF4根据在火星上飞行时的正常冲击密度比为12来模拟大约为12的马赫数。该实验研究的结果表明,当无法为此类行星进入车辆提供空气动力学装饰的传统方法(例如,偏置等)时,单个襟翼可以提供相似的空气动力学性能。通过在可比雷诺数下的6马赫理想空气中进行协同测试,获得了归因于真实气体的钝体空气动力效应的评估。从空气动力学的角度来看,已发现适当尺寸的襟翼可在所需的升阻比下提供足够的修剪能力,以实现精确着陆。进行了使用非结构化网格的无粘性高超声速流动计算,以评估襟翼的可行性,从而为Lander提供空气动力学的内饰。随后的Navier-Stokes计算预测与实验测量非常吻合。

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