首页> 外文会议>International Solar Cycle Studies (ISCS) Symposium 2003; Jun 23-28, 2003; Tatranska Lomnica, Slovak Republic >RELATIONSHIP BETWEEN SOLAR RADIO SPIKES OBSERVED AT 1420 MHZ AND SOLAR ACTIVE PHENOMENA
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RELATIONSHIP BETWEEN SOLAR RADIO SPIKES OBSERVED AT 1420 MHZ AND SOLAR ACTIVE PHENOMENA

机译:在1420 MHZ观察到的太阳辐射峰值与太阳活动现象之间的关系

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Numerous solar radio narrow-band spikes have been observed with the RT-15 radio telescope of Torun Observatory between March 15, 2000 and May 14, 2001. We present here a brief description of three interesting events (from 11 events collected during 2000 hours of observations) and first results of analysis of the relationship between the spikes, solar flares and coronal mass ejections. We have found that solar spikes were emitted from solar flares of various scenario of evolution and various configuration of the interacting magnetic fields. Moreover, some groups of spikes were not correlated in time with any solar flare recorded by GOES or Yohkoh. It is very interesting to note, that on the basis of the GOES database merely 2% of the solar flares emit the radio spikes.
机译:在2000年3月15日至2001年5月14日之间,托伦天文台的RT-15射电望远镜观测到许多太阳射电窄带尖峰信号。在此,我们简要介绍三个有趣的事件(从2000年以来收集的11个事件观测结果)以及分析尖峰,太阳耀斑和日冕物质抛射之间关系的第一个结果。我们发现,太阳峰是从各种演化情况和相互作用磁场的各种配置的太阳耀斑发出的。而且,一些峰值与时间没有与GOES或Yohkoh记录的任何太阳耀斑相关。值得注意的是,在GOES数据库的基础上,仅有2%的太阳耀斑发射了无线电波尖峰。

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