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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

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【作者】 黄宇黄光力

【Author】 Huang Yu1,2,Huang Guangli1(1.Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China,2.Graduate University of the Chinese Academy of Sciences,Beijing 100049,China)

【机构】 中国科学院紫金山天文台中国科学院研究生院

【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.

【基金】 国家自然科学基金(11073058)资助
  • 【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
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