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The aerodynamics of axisymmetric blunt bodies flying at angle of attack

机译:轴对称钝体以迎角飞行的空气动力学

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The Mars Science Laboratory entry capsule is used as an example to demonstrate how a blunt body of revolution must be treated as asymmetric in some respects when flying at a non-zero trim angle of attack. A brief description of the axisymmetric moment equations are provided before solving a system of equations describing the lateral-directional moment equations for a blunt body trimming at an angle of attack. Simplifying assumptions are made which allow the solution to the equations to be rearranged to relate the roll and yaw stability with sideslip angle to the frequency of oscillation of the vehicle body rates. The equations show that for a blunt body the roll and yaw rates are in phase and proportional to each other. The ratio of the rates is determined by the static stability coefficients and mass properties about those axes. A trajectory simulation is used to validate the static yaw stability parameter identification equation and a simple method of identifying the oscillation frequency from the body rates. The approach is shown to successfully extract the modeled yaw stability coefficient along a simulated Mars entry. Mars Science Laboratory flight data results are presented from earlier work which indicate that results from both the validation case and flight data are in agreement with preflight predictions. A brief discussion of the dynamic stability is also provided. Trimming at a nonzero angle suggests that the typical axisymmetric models of the dynamic stability coefficients should be modified. However, further experimental or computational work must be done to separate damping due to body rates and wind relative rates before the correct lifting formulation would affect simulation results.
机译:以火星科学实验室的入口舱为例,以说明在非零纵倾角飞行时,钝头旋转体在某些方面必须被视为不对称。在求解方程组之前,先对轴对称矩方程进行简要说明,该方程组描述了在迎角处钝体修整的横向矩方程。做出简化的假设,可以重新安排方程式的求解,以将侧滑角的侧倾和偏航稳定性与车速的振荡频率相关联。这些方程式表明,对于钝性车身,侧倾和偏航率是同相且彼此成比例的。比率的比值由这些轴的静态稳定性系数和质量特性决定。使用轨迹模拟来验证静态偏航稳定性参数识别方程,以及一种从人体速率识别振荡频率的简单方法。结果表明,该方法成功地沿模拟火星入口提取了模型的偏航稳定性系数。火星科学实验室的飞行数据结果来自早期工作,表明验证案例和飞行数据的结果均与飞行前的预测相符。还提供了动态稳定性的简短讨论。以非零角度修整表明,应修改动力稳定性系数的典型轴对称模型。但是,在正确的提升公式会影响模拟结果之前,必须进行进一步的实验或计算工作以分离由于车速和相对风速引起的阻尼。

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