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Numerical Simulation of control of plasma flow with magnetic field for thermal protection in Earth reentry flight

机译:再入飞行中热保护磁场控制等离子体流的数值模拟。

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The present numerical study examines the possibility and usefulness of the control of weakly ionized plasma flow ahead of a space vehicle by means of the magnetic field for thermal protection in earth reentry flight under the flight conditions at the altitudes from about 72 to 48 km along the real earth reentry trajectory of the blunt body OREX, which was used for an earth reentry experiment in 1994. Numerical results show that the aerodynamic heating can be reduced by applying the magnetic field at the altitude above about 55 km where the weakly ionized plasma is produced behind the bow shock wave, and also that the reduction amount of the aerodynamic heating by applying the magnetic field becomes larger with increasing the altitude. At the altitude of about 60 km, where the aerodynamic heating had the peak value in the OREX experiment, the wall heat flux at the stagnation point and the total aerodynamic heating over the wall surface with applying the magnetic field of about 0.5 T are, respectively, 85% and 67% of their values obtained without applying the magnetic field.
机译:目前的数值研究探讨了在磁场重载飞行中,在沿海拔约72至48 km的飞行条件下,利用磁场进行热保护的方法,可以控制航天器前方弱电离等离子体流的可能性和有用性。钝体OREX的真实地球折返轨迹,1994年用于一次地球折返实验。数值结果表明,通过在高于55 km的海拔处产生弱电离等离子体的磁场施加磁场,可以降低空气动力加热而且,随着高度的增加,通过施加磁场引起的空气动力加热的减少量变大。在OREX实验中空气加热达到峰值的约60 km高度处,在施加约0.5 T磁场的情况下,驻点处的壁热通量和壁表面上的总空气动力学热分别为,它们的值的85%和67%无需施加磁场即可获得。

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