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Effects of thermal radiation heat transfer on flame acceleration and transition to detonation in particle-cloud flames

机译:热辐射传热对火焰加速和燃烧的影响   过渡到粒子云火焰中的爆炸

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摘要

The current work examines regimes of the hydrogen-oxygen flame propagationand ignition of mixtures heated by radiation emitted from the flame. Thegaseous phase is assumed to be transparent for the radiation, while thesuspended particles of the dust cloud ahead of the flame absorb and reemit theradiation. The radiant heat absorbed by the particles is then lost byconduction to the surrounding unreacted gaseous phase so that the gas phasetemperature lags that of the particles. The direct numerical simulations solvethe full system of two phase gas dynamic time-dependent equations with adetailed chemical kinetics for a plane flames propagating through a dust cloud.It is shown that depending on the spatial distribution of the dispersedparticles and on the value of radiation absorption length the consequence ofthe radiative preheating of the mixture ahead of the flame can be either theincrease of the flame velocity for uniformly dispersed particles or ignitioneither new deflagration or detonation ahead of the original flame via theZel'dovich gradient mechanism in the case of a layered particle-gas clouddeposits. In the latter case the ignited combustion regime depends on theradiation absorption length and correspondingly on the steepness of the formedtemperature gradient in the preignition zone that can be treated independentlyof the primary flame. The impact of radiation heat transfer in a particle-ladenflames is of paramount importance for better risk assessment and represents aroute for understanding of dust explosion origin.
机译:当前的工作研究了氢-氧火焰传播和由火焰发射的辐射加热的混合物着火的机制。假定气相对辐射是透明的,而在火焰之前的尘埃云悬浮颗粒吸收并重新辐射。然后,被颗粒吸收的辐射热通过与周围未反应的气相传导而损失掉,从而使气相温度落后于颗粒的气相温度。直接数值模拟解决了两相气体动力学随时间变化的方程的完整系统,该方程具有详细的化学动力学,用于传播穿过尘埃云的平面火焰,结果表明,这取决于分散粒子的空间分布和辐射吸收长度的值混合物在火焰之前进行辐射预热的结果可能是均匀分散颗粒的火焰速度增加,或者在颗粒气体分层的情况下,通过Zel'dovich梯度机理在原始火焰之前点燃了新的爆燃或引爆云沉积。在后一种情况下,点燃的燃烧方式取决于辐射吸收长度,并且相应地取决于可独立于一次火焰处理的,在提前点火区内形成的温度梯度的陡度。辐射热在颗粒状火焰中的影响对于更好的风险评估至关重要,是理解粉尘爆炸起源的途径。

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