Kinetic Modelling of Atmospheric Pressure Nitrogen Plasma

M. Rahman, Mohammed Mynuddin
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引用次数: 11

Abstract

This model describes the production and destruction mechanism of nitrogen plasma at atmospheric pressure. We have studied the mechanisms of chemical dissociation, ionization, ion conversion and recombination in nitrogen plasmas, with kinetic temperature ( T g ) of the free electrons being higher than the kinetic temperature ( T g ) of heavy species. Therefore, the investigation of nitrogen plasma species in a wide range of pressure from 1 Torr to 760 Torr is interesting phenomena for obtaining the equilibrium state when the nitrogen species breakdown. In order to calculate the species densities to reach thermodynamic equilibrium under various conditions, a set of chemical kinetic reactions of nitrogen under consideration have been simulated. It solves the particle balance equations for a set of interacting species. In this study 16 reactions and 4 species of Nitrogen N, N 2 , N + , N 2 + and electron have been considered. The densities of the charged and neutral species are modeled by continuity equations which includes the relevant plasma-chemical kinetics. Nitrogen species density is guided by continuity equation where chemical processes and Arrhenius form are used to follow the change of species density over the time. To calculate the species densities over pressure, temperature and time the continuity equations of the 16 reactions for the 5 species under consideration giving their initial pressure, densities and temperatures, with the latter held constant have been solved. The variations of species densities have been investigated as a function of pressure ranging from 1 to 760 Torr. This model shows that as the pressure is increased the species densities of nitrogen plasma also increase from pressure 1 to 200 Torr and after pressure above 200 Torr the species densities become almost saturated. The change of species densities at various temperatures ranging from 2000 Kelvin to 25000 Kelvin is successfully investigated. The destruction and production rates of the nitrogen species also have been calculated within the time ranging from 0 to 19nS and it shows that the density of nitrogen plasma increases with time. In our study we have considered the gas and electron temperature as 10k Kelvin and 4eV respectively.
大气压氮等离子体的动力学模拟
该模型描述了大气压力下氮等离子体的产生和破坏机理。我们研究了氮等离子体中化学解离、电离、离子转化和复合的机理,其中自由电子的动力学温度(T g)高于重物质的动力学温度(T g)。因此,在1 ~ 760托的大压力范围内研究氮等离子体种是获得氮种击穿时平衡态的有趣现象。为了计算在不同条件下达到热力学平衡的物质密度,模拟了一组氮气的化学动力学反应。它解决了一组相互作用物种的粒子平衡方程。本研究考虑了16种反应和4种氮(N、n2、N +、n2 +和电子)。带电和中性物质的密度用包含相关等离子体化学动力学的连续性方程来模拟。氮的物种密度以连续性方程为指导,利用化学过程和阿伦尼乌斯形式来跟踪物种密度随时间的变化。为了计算物质密度随压力、温度和时间的变化,在初始压力、密度和温度不变的情况下,求解了16种反应中5种物质的连续方程。物种密度的变化已经作为压力范围从1到760托的函数进行了研究。该模型表明,随着压力的增加,氮等离子体的物种密度也从压力1增加到200 Torr,当压力超过200 Torr时,物种密度几乎饱和。成功地研究了在2000 ~ 25000开尔文温度范围内物质密度的变化。在0 ~ 19nS的时间内计算了氮的破坏速率和生成速率,结果表明氮等离子体的密度随时间的增加而增加。在我们的研究中,我们认为气体和电子温度分别为10k开尔文和4eV。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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