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太阳射电辐射的自调制模型
引用本文:黄光力,毛定一.太阳射电辐射的自调制模型[J].天文学报,1997,38(4):379-385.
作者姓名:黄光力  毛定一
作者单位:中国科学院紫金山天文台!南京,210008,中国科学院紫金山天文台!南京,210008,河海大学数理系!南京,210024
摘    要:本文采用几何光学近似,研究在日冕条件下,沿着磁场传播的电磁波产生非线性自调制不稳定性的可能.发现只有分米波和米波段的射电爆发,可以在日冕外层产生纵向和横向的自调制不稳定性.而在其它波段,如光学、X射线和高频电磁波,则不会产生这样的非线性不稳定性过程.由纵向自调制不稳定性产生的精细结构具有包络孤波的形状.

关 键 词:太阳射电  非线性过程  波的调制

A SELF-MODULATION MODEL OF SOLAR RADIO EMISSION
Wang De-yu, Huang Guang-li.A SELF-MODULATION MODEL OF SOLAR RADIO EMISSION[J].Acta Astronomica Sinica,1997,38(4):379-385.
Authors:Wang De-yu  Huang Guang-li
Abstract:The existing theorehcal model of self-modulation instability in the nonlinear wavespropagation is adopted in thes work. We want to investigate the possibility ofself-modulation instablities occurring in the electromagnetic waves propagating in thesolar corona. It is found that only decimeter and meter radio bursts can produce thelongitudinal and transverse self-modulation instabilities in the outer corona and that theoptical, X-ray and high frequency electromagnetic waves are unable to produce suchmodulation processes. This theoretical model is consistent with the observed finestructures of solar meter wave bursts.
Keywords:solar radio emission  nonlinear process  wave modulation
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