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Determination of Temperature Profiles in the Plenum Region of the NASA IHF Arc Jet Facility from Emission Spectroscopic Measurements

机译:通过发射光谱测量确定NASA IHF电弧射流设施全区温度曲线

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Emission spectroscopy data taken in the plenum of the NASA Ames 60 MW Interaction Heating Facility (IHF) were analyzed to validate best practices for determining an inflow condition for CFD simulation of the arc-jet flow. Previously, data analysis was performed through a comparison of the experimental spectra with simulated ones based on the existing CFD simulation. In this work, an equilibrium chemistry data base is built and used to generate a spectral database for relevant temperatures and pressures. Through iteration of plasma conditions matching the experimental data at different offset positions, radial profiles of equilibrium temperatures were obtained characterizing the local specific enthalpy in the plenum. This method has the advantage of being independent from any modeling assumption (except the justifiable assumption of equilibrium conditions). In a first step, the temperature profiles were iterated manually. For this purpose, the plenum was divided in a number of rings with constant compositions and temperatures, according to the number of lines of sight available from the experimental data. In parallel, a method for automatically fitting these conditions through Fortran code was developed. Both methods were found to agree and were able to fit the measured data. In comparison to the CFD solution, the temperature profiles obtained in this work showed significantly higher temperatures at the center line of the plenum, but lower values close to the wall. Therefore, the plasma beam seems to form a hot core region with a distinct temperature profile. Furthermore, these preliminary results indicate that current practices of assuming a swirl flow with reduced static pressures at the center line of the plenum seems to be inappropriate. Future work will include a statistic analysis of repeated measurements of the same plasma condition, as well as parametric investigations of possible pressure distributions inside the plenum region and continuous temperature distributions along the plenum radius.
机译:分析了在NASA Ames 60 MW互动加热设施(IHF)的气室中获得的发射光谱数据,以验证确定CFD模拟电弧射流的入流条件的最佳做法。以前,数据分析是通过将实验光谱与基于现有CFD模拟的模拟光谱进行比较来进行的。在这项工作中,建立了一个平衡化学数据库,并用于生成有关温度和压力的光谱数据库。通过在不同偏移位置匹配实验数据的等离子体条件的迭代,获得了平衡温度的径向曲线,该径向温度表征了气室中的局部比焓。该方法的优点是独立于任何建模假设(平衡条件的合理假设除外)。第一步,温度曲线是手动迭代的。为此,根据可从实验数据获得的视线数量,将气室分成具有恒定成分和温度的多个环。同时,开发了一种通过Fortran代码自动拟合这些条件的方法。两种方法都被认为是一致的,并且能够拟合所测得的数据。与CFD解决方案相比,在这项工作中获得的温度曲线显示,气室中心线的温度明显较高,但靠近壁的温度较低。因此,等离子束似乎形成了具有明显温度分布的热芯区域。此外,这些初步结果表明,当前的假设做法是在增压室中心线处采用减小的静压的涡流进行似乎是不合适的。未来的工作将包括对相同血浆条件的重复测量进行统计分析,以及对气室区域内可能的压力分布以及沿气室半径的连续温度分布进行参数研究。

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