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Comment on “Locating the source field lines of Jovian decametric radio emissions” by YuMing Wang et al.

Abstract : In this comment on the article "Locating the source field lines of Jovian decametric radio emissions" by Wang YM 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 14 th March 2014 by Wind and both STEREO A/B spacecraft from ~5 to ~16 MHz. They have erroneously identified the emission as a northern (Io-B type) instead of a southern one (Io-D type). We encourage the authors to update their results with the correct hemisphere of origin and to test their method on a larger sample of Jupiter-Io emissions.
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https://hal-obspm.ccsd.cnrs.fr/obspm-03684603
Contributor : Baptiste Cecconi Connect in order to contact the contributor
Submitted on : Wednesday, June 8, 2022 - 3:19:06 PM
Last modification on : Friday, August 5, 2022 - 12:00:55 PM
Long-term archiving on: : Friday, September 9, 2022 - 6:33:22 PM

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Laurent Lamy, Baptiste Cecconi, Stéphane Aicardi, Corentin K. Louis. Comment on “Locating the source field lines of Jovian decametric radio emissions” by YuMing Wang et al.. Earth and Planetary Physics, Science Press., 2022, 6 (1), pp.10 - 12. ⟨10.26464/epp2022018⟩. ⟨obspm-03684603⟩

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