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Study of Earth and Jupiter-like plasmas for atmospheric entries using a non-transferred arc torch

机译:用非转移弧焊炬研究地球和木星等离子进入大气

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This paper presents the results obtained by a 100 kW non-transferred arc plasma torch dedicated to the studies of plasmas characteristics of atmospheric entries of spatial probes, especially Earth and Jupiter entries. Spectra acquisition of the produced plasmas is achieved using optical emission spectroscopy. For Earth entry conditions, air plasma was obtained with a maximal temperature around 6800 K with a good agreement using atomic lines of oxygen and nitrogen (and also copper coming from electrode's ablation) and molecular bands of N-2, CN and N-2+, testifying to a good thermal equilibrium. As the first step in the study of Jupiter atmospheric entry, pure helium plasma was produced with the same maximal temperature of about 7500 K. Helium plasma was achieved for the first time using the plasma torch. Recorded spectra show a continuum, He I lines as well as copper. He II lines are not detected.
机译:本文介绍了由100 kW非转移弧等离子炬获得的结果,该炬专门用于研究空间探针(尤其是地球和木星)大气入口的等离子体特征。产生的等离子体的光谱采集是使用光发射光谱法实现的。对于地球进入条件,使用氧气和氮气(以及来自电极烧蚀的铜)和N-2,CN和N-2 +的分子带原子线,获得了最高温度约为6800 K的良好协议的空气等离子体。证明了良好的热平衡。作为研究木星进入大气层的第一步,以相同的最高温度约7500 K产生纯氦等离子体。使用等离子炬首次实现了氦等离子体。记录的光谱显示出一个连续的,He I线以及铜。未检测到He II线。

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