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Ignition of Deflagration and Detonation Ahead of the Flame due to Radiative Preheating of Suspended Micro Particles

机译:火焰爆炸引发的爆燃和爆轰点火   悬浮微粒的辐射预热

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摘要

We study a flame propagating in the gaseous combustible mixture withsuspended inert particles. The gas is assumed to be transparent for theradiation emitted by the combustion products, while particles absorb andre-emit the radiation. Thermal radiation heats the particles, which in turntransfer the heat to the surrounding gaseous mixture by means of heatconduction, so that the gas temperature lags that of the particles. We considerdifferent scenarios depending on the spatial distribution of the particles,their size and the number density. In the case of uniform distribution of theparticles the radiation causes a modest increase of the temperature ahead ofthe flame and the corresponding increase of the flame velocity. The effects ofradiation preheating is stronger for a flame with smaller normal velocity. Inthe case of non-uniform distribution of the particles, such that the particlesnumber density is smaller just ahead of the flame and increases in the distantregion ahead of the flame, the preheating caused by the thermal radiation maytrigger additional independent source of ignition. This scenario requires theformation of a temperature gradient with the maximum temperature sufficient forignition in the region of denser particles cloud ahead of the advancing flame.Depending on the steepness of the temperature gradient formed in the unburnedmixture, either deflagration or detonation can be initiated via the Zeldovich'sgradient mechanism. The ignition and the resulting combustion regimes depend onthe temperature profile which is formed in effect of radiation absorption andgas-dynamic expansion. In the case of coal dust flames propagating through alayered dust cloud the effect of radiation heat transfer can result in thepropagation of combustion wave with velocity up to 1000m/s and can be aplausible explanation of the origin of dust explosion in coal mines.
机译:我们研究了在带有悬浮惰性粒子的气态可燃混合物中传播的火焰。假定气体对燃烧产物发出的辐射是透明的,而颗粒则吸收并重新发射辐射。热辐射加热颗粒,然后通过热传导将热量传递到周围的气体混合物中,从而使气体温度落后于颗粒的温度。我们根据粒子的空间分布,大小和数量密度来考虑不同的情况。在颗粒均匀分布的情况下,辐射导致火焰之前的温度适度增加,并且火焰速度相应增加。对于法向速度较小的火焰,辐射预热的影响更大。在颗粒分布不均匀的情况下,使得颗粒数量密度正好在火焰之前较小,而在火焰之前的较远区域则增加,由热辐射引起的预热可能会触发额外的独立点火源。在这种情况下,需要形成一个温度梯度,使最高温度在燃烧火焰之前的致密颗粒云区域中具有足够的点火能力,这取决于未燃烧混合物中形成的温度梯度的陡度,可以通过Zeldovich引发爆燃或爆炸的梯度机制。点火和产生的燃烧状态取决于在辐射吸收和气体动力膨胀的作用下形成的温度曲线。在煤尘火焰通过层层尘埃云传播的情况下,辐射传热的作用可以导致燃烧波以高达1000m / s的速度传播,并且可以合理解释煤尘爆炸的起源。

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