高速飞行器紫外辐射模型建立与特征分析

Modeling and Characteristics of ultraviolet radiation from high-speed vehicles

  • 摘要: 高速飞行器的探测是航空航天工作的重点,其辐射波段范围涉及紫外、可见光和红外等区域。目前对于激波层辐射特性的研究主要集中在红外辐射区域,较少关注紫外辐射特性。针对上述问题,为提供飞行器探测的最优波段范围,本研究建立了一个综合框架,用于分析临近空间条件下的气体辐射特性,结合计算流体动力学和量子辐射物理学,阐明高速飞行器的紫外线光谱特征;辐射场采用混合增宽方式和逐线计算方法的三温模型计算;此外,采用了一种多尺度模拟方法,将直接模拟蒙特卡罗(DSMC)粒子方法与量子动力学建模相结合;并对H = 60、70、75 km的高速飞行器流场进行紫外波段辐射强度模拟。本文得出以下结论:平衡态时,紫外波段光谱辐射强度随温度升高而升高;非平衡态时,随着振动温度Tv、电子温度Te的降低,紫外波段光谱辐射强度逐渐降低;紫外波段辐射强度除与温度相关外,还与分子数密度相关,且与NO和O2的关系较为密切;紫外辐射最强区位于飞行器下腹,辐射峰值位置随高度迁移。

     

    Abstract: The rapid advancement of near-space hypersonic vehicles, including air-breathing cruise missiles, strategic glide vehicles, hypersonic boost-glide vehicles, and space-to-ground platforms, has created an urgent need for advanced detection technologies and thermal protection solutions. Traditional radars are increasingly ineffective against next-generation stealth-capable hypersonic targets, while conventional infrared detection remains constrained by an incomplete understanding of complex radiation mechanisms. Despite extensive research into thermal emissions from vehicle surfaces and flow fields, a significant knowledge gap remains concerning the critical domain of shock wave-induced short-wave radiation, particularly in extreme flight regimes. Addressing these challenges requires coordinate advances in detection technology and thermal management strategies. This study presents a comprehensive framework for analyzing gas radiation characteristics in near space (altitudes ≥20 km, Mach numbers ≥10), which integrates a multiscale simulation approach combining Direct simulation Monte Carlo (DSMC) with quantum-kinetic modeling. Radiation fields are computed using a three-temperature model (translational, vibrational, and electronic) that incorporates line-by-line spectral resolution and line-of-sight integration. A systematic investigation of radiation patterns in representative hypersonic flow fields, reveals that the equilibrium ultraviolet radiation intensity demonstrates exponential temperature dependence, while non-equilibrium states exhibit complex coupling between vibrational/electronic excitation temperatures and translational energy modes. Moreover, ultraviolet emission profiles show a strong correlation with molecular number density, particularly those of nitric oxide (NO) and diatomic oxygen (O2), which dominate radiative processes in high-enthalpy flows. Counterintuitively, the maximum radiation intensity does not occur near the nose tip, as in the region of peak heating, but at the ventral stagnation point during high-angle-of-attack maneuvers. These results shed light on optimizing detector wavelengths and designing thermal protection systems for next-generation hypersonic vehicles.

     

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