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用网格粒子数值模拟方法研究反向Langmuir波的产生机制
Study of Backward-Propagating Langmuir Waves with Numerical Simulations Based on the Particle-in-Cell Method
【摘要】 一般认为,Langmuir波(LW)转换为电磁波是太阳Ⅲ型射电爆的产生机制。由电子束流不稳定性可以很容易地激发LW,正向LW和反向LW的相互作用被认为是产生Ⅲ型爆二次谐波的原因,但反向LW的色散方程和产生机制尚未得到充分研究。通过粒子(Particle In Cell,PIC)模拟研究了反向LW的产生机制,发现反向LW不能由电子束流直接激发,其能量基本上是由正向LW散射得到的。然而,电子束流对正向LW的二次谐波有直接放大作用。
【Abstract】 The conversion of Langmuir waves into electromagnetic radiations is an important mechanism of Type Ⅲ solar bursts.Langmuir Waves(LW) can be easily excited by electron-beam instabilities,and they can become backward propagating throuth the wave-wave interaction.Generally,the backward-propagating LW are very important for the second-harmonic waves of Type Ⅲ solar bursts.In this paper we pay particular attention to the mechanism of the backward-propagating LW as revealed through numerical simulations based on the Partical-in-Cell(PIC) method.We found that ions play a key role to excite the backward-propagating LW,with draw much of their energy from the scattering of the forward-propagating LW.Moreover,an electron beam can hardly generate backward-propagating LW directly,but may directly amplify second-harmonic forward-propagating LW.
【Key words】 Langmuir wave; Simulation with PIC; Backward propagating; Type Ⅲ bursts;
- 【文献出处】 天文研究与技术 ,Astronomical Research & Technology , 编辑部邮箱 ,2012年04期
- 【分类号】P182.2
- 【下载频次】36