期刊文献+

太阳射电分米波毫秒级尖峰辐射的寿命

Duration of the Solar Radio Spike Radiation at Decimetric Waves and Milliseconds
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摘要 太阳射电毫秒级尖峰辐射的寿命随频率增高而减小,长期以来这一直是个令人困惑的问题。本文从与Ⅲ型爆发相关的空心束分布的电子流所激发的回旋同步脉泽角度出发,详细讨论了尖峰辐射的寿命与特征频率比(ξ=ω_P/ω_B)以及波增长率的关系,最后得出:在分米波的不同波段,尖峰辐射是X模的不同次谐波,且寿命随频率增高发生相关的减小。 The duration of the solar radio millisecond spike radiation is shortened with the increase in the frequency,which has been a puzzling problem for a long time.In this paper,according to the electron cyclotron maser excited by the electron beams of the hollow beam distribution associated with the type Ⅲ bursts,the relation between the duration of the spike radiation and the characteristic frequency ratio(i.e.the parameter = ψp /ψB)with the wave growth rate is discussed in detail.Finally,it is concluded that at the different wavelengths of the decimetric wave,the spike radiations are the different frequency harmonic waves and the correlative decrease of the duration appears with the increase in the frequency.
出处 《云南天文台台刊》 CSCD 1993年第3期24-28,共5页 Publications of the Yunnan Observatoty
关键词 寿命 辐射 尖峰辐射 太阳 射电爆发 Solar radio burst Spike radiation
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参考文献4

  • 1曹文达.太阳射电分米波尖峰辐射和米波射电爆发[J].云南天文台台刊,1992(3):8-18. 被引量:1
  • 2李春生,傅其骏,严玉华,江淑英,李宏为.耀斑脉冲相微波毫秒级尖峰辐射及其共生现象[J]Chinese Journal of Astronomy and Astrophysics,1985(01).
  • 3A. O. Benz. Millisecond radio spikes[J] 1986,Solar Physics(1):99~110
  • 4Hong Wei Li. Hollow beam distribution of energetic electrons and higher harmonics of electron cyclotron maser[J] 1986,Solar Physics(1):131~136

二级参考文献6

  • 1谢瑞祥,杨开平,李维华,陈国强,马媛,张帆,赵日昇.三波段太阳射电高时间分辨率同步观测系统的研制[J].天体物理学报,1989,9(1):77-83. 被引量:5
  • 2李春生,郑兴武,江淑英,姚金兴,周爱华.太阳射电IV型爆发U形谱的产生机制[J]天文学报,1979(02).
  • 3Shuchen Ji,Ruixiang Xie,Wang Min. Millisecond radio spikes on long centimetre and short decimetre wavelengths and occurrence frequency[J] 1992,Astrophysics and Space Science(1):33~41
  • 4R. M. Winglee,G. A. Dulk. Electron-cyclotron maser emission from the sun and stars: Variations with plasma temperature and density[J] 1986,Solar Physics(1):93~97
  • 5A. O. Benz. Millisecond radio spikes[J] 1986,Solar Physics(1):99~110
  • 6M. Karlicky. Narrowband dm-spikes as indication of flare mass ejection[J] 1984,Solar Physics(1-2):329~342

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