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Statistical Survey of Type III Radio Bursts at Long Wavelengths Observed by the Solar TErrestrial RElations Observatory (STEREO)/Waves Instruments: Radio Flux Density Variations with Frequency

机译:太阳地面关系天文台(STEREO)/波仪器观测到的长波长III型无线电爆发的统计调查:无线电通量密度随频率的变化

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摘要

We have performed a statistical study of 152 Type III radio bursts observed by Solar TErrestrial RElations Observatory (STEREO)/Waves between May 2007 and February 2013. We investigated the flux density between 125 kHz and 16 MHz. Both high- and low-frequency cutoffs were observed in 60 % of events, suggesting an important role of propagation. As already reported by previous authors, we observed that the highest flux density occurs at 1 MHz on both spacecraft. We developed a simplified analytical model of the flux density as a function of radial distance and compared it with the STEREO/Waves data.
机译:我们已对2007年5月至2013年2月之间的太阳地面关系观测站(STEREO)/波观测到的152个III型无线电脉冲进行了统计研究。我们研究了125 kHz至16 MHz之间的通量密度。在60%的事件中都观察到了高频和低频截止,表明传播具有重要作用。正如以前的作者已经报道的那样,我们观察到两个航天器的最高通量密度都出现在1 MHz处。我们开发了通量密度随径向距离变化的简化分析模型,并将其与STEREO / Waves数据进行了比较。

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