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Discharge mechanims of sub-microsecond pulsed atmospheric pressure glow discharges

机译:亚微秒大气压脉冲辉光放电的放电机理

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Nonthermal atmospheric pressure plasmas have attracted much attention for their convenient applications on surface modifications, thin film deposition, biological sterilization and inactivation et al. Most atmospheric pressure glow discharges (APGDs) are generated by sinusoidal excitation with repetition frequency from kilo hertz to mega hertz. Recently, high voltage pulses with duration less than one microsecond are apply for APGDs, which demonstrated the reduced discharge power consumption and improved discharge stability even without dielectric barriers. Currently, the understanding of discharge mechanism in terms of gas breakdown and discharge evolution are still limited due to the ultra-fast (sub-microsecond) temporal evolution of discharge, which restricts the experimental diagnostics. [1,2] Here, a one-dimensional fluid model was developed for numerical studies of pulsed APGDs.
机译:非热大气压等离子体由于其在表面改性,薄膜沉积,生物灭菌和灭活等方面的便利应用而受到广泛关注。大多数大气压辉光放电(APGD)是由正弦激励产生的,其重复频率从千赫兹到兆赫兹。最近,持续时间小于一微秒的高压脉冲被应用于APGD,这证明了降低的放电功率消耗和改善的放电稳定性,即使没有介电阻挡层也是如此。目前,由于放电的超快速(亚微秒)时间演变,对气体分解和放电演变方面的放电机理的理解仍然受到限制,这限制了实验诊断。 [1,2]在这里,开发了一维流体模型用于脉冲APGD的数值研究。

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