论文标题
评论Yuming Wang等人的“定位Jovian DeTametric Radio排放的源场线”
Comment on "Locating the source field lines of Jovian decametric radio emissions" by YuMing Wang et al
论文作者
论文摘要
在Yuming Wang等，2020年的文章[Arxiv：2002.01150]的这篇评论中，“定位Jovian Decametric Radio排放的源场线”，我们讨论了作者用于计算Moon IO所指出的Jupiter S decametric sematemetrics dematectric secametric secaming角的假设。他们的方法依赖于多点无线电观测，将Wind于2014年3月14日在2014年3月14日观察到的单一事件，以及立体声A/B航天器的5至16 MHz，并错误地识别为北部发射（IO-B类型），而不是南部发射（IO-D类型）（IO-D类型）。我们鼓励作者使用原始的正确半球更新其结果，并在更大的木星-IO排放样本上测试其方法。
In this comment of the article [arXiv:2002.01150] "Locating the source field lines of Jovian decametric radio emissions" by YuMing Wang et al., 2020, we discuss the assumptions used by the authors to compute the beaming angle of Jupiter s decametric emissions induced by the moon Io. Their method, relying on multi-point radio observations, was applied to a single event observed on 14th March 2014 by Wind and both STEREO A/B spacecraft from 5 to 16 MHz, and erroneously identified as a northern emission (Io-B type) instead of a southern one (Io-D type). We encourage the authors to update their results with the right hemisphere of origin and to test their method on a larger sample of Jupiter-Io emissions.
