期刊文献+

太阳射电短厘米波精细结构的非线性调制模型

A NON-LINEAR MODULATION MODEL FOR THE FINE STRUCTURES IN THE SOLAR SHORT CENTIMETRE WAVE BURSTS
下载PDF
导出
摘要 本文提出一种理论模型:认为太阳短厘米波射电辐射在通过日冕时,可与目冕中的MHD波发生三波共振相互作用,辐射流量会产生非线性调制.这种模型可以很好地解释观测到的精细结构中流量与重复率的反比例关系.而且,理论预期调制周期与射电频率有关,精细结构的调制幅度与射电流量无关. A theoretical model has been suggested hee. The three-waves resonance interaction can occur when this radio emission interacts with the MHD wave in the corona, while the short centimetre emission from solar radio bursts passes through the corona. These induce a non-linear modulation of the emission flux. This model can satisfactorily interpret the inversely proportional relation between the observed flux and the repetition rates of fine structures in the solar short centimetre wave bursts. Moreover, this theoretical model anticipates that the modulation period is related to the radio frequency, while the modulated amplitude of the fine structures is independent of the radio flux.
作者 王德焴
出处 《天文学报》 CSCD 北大核心 1991年第4期362-368,共7页 Acta Astronomica Sinica
关键词 太阳 射电 精细结构 调制 fine structure in solar radio bursts—wave modulation
  • 相关文献

参考文献3

  • 1王德Yu,Solar Phys,1991年
  • 2秦志海,天文学报,1991年,32卷,3页
  • 3匿名著者,非线性波动,1981年

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部