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UV- and IR-Signatures of Rocket Plumes

机译:火箭羽的紫外和红外特征

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Spectral characteristics of ultraviolet and infrared rocket plume signatures are of great importance especially for detection, identification and tracking of approaching missiles. The objective was to find out significant differences between plume signatures of available real rocket motors based on double base and composite propellants. Therefore, the spectral emission ranges of 305 - 385 nm (UV) and 1.7 - 14 #mu#m (MIR) were measured from the head-on aspect. Additionally, reaction processes of applied propellant compositions were calculated by the ICT Thermodynamic-Code and taken for the simulation of the theoretical spectra based on the ICT Band Modeling-Code (BAM).
机译:紫外和红外火箭羽流特征的光谱特性非常重要,特别是对于探测,识别和跟踪接近的导弹。目的是找出基于双基和复合推进剂的实际火箭发动机的羽流特征之间的显着差异。因此,从正面角度测量的光谱发射范围为305-385 nm(UV)和1.7-14#mu#m(MIR)。此外,通过ICT热力学代码计算了所施加推进剂成分的反应过程,并根据ICT波段建模代码(BAM)将其用于理论光谱的仿真。

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