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Preliminary Analysis of a Joint Observation of the Complex Solar Radio Burst of 1998 September 23

机译:对1998年9月23日复杂太阳射电爆发联合观测的初步分析。

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摘要

We have carried out a preliminary comparative analysis of a large, complex, type III-IV solar burst observed on 1998-09-23 with the 1-2 GHz and 2.6-3.8 GHz spectrometers of Beijing Astronomical Observatory as well as with the Russian SSRT and the German decimetric-metric dynamical spectrometer. The contents for research on the acceleration of electrons in the solar corona and on the structure of coronal magnetic field have been extended. Some observed phenomena and the radiation mechanisms of moving type IV bursts and multiple pulsations are briefly interpreted.
机译:我们对北京天文台1-2 GHz和2.6-3.8 GHz光谱仪以及俄罗斯SSRT于1998-09-23观测到的大型,复杂的III-IV型太阳爆发进行了初步比较分析。和德国的动态计量分光仪。关于日冕中电子加速和日冕磁场结构的研究内容已经扩展。简要解释了一些观察到的现象以及IV型脉冲和多脉冲运动的辐射机理。

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