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ISSN  2096-3955

CN  10-1502/P

Citation: Lamy, L., Cecconi, B., Aicardi, S., and Louis, C. K. (2022). Comment on “Locating the source field lines of Jovian decametric radio emissions” by YuMing Wang et al.. Earth Planet. Phys., 6(1), 10–12.

2022, 6(1): 10-12. doi: 10.26464/epp2022018


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


LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France


Station de Radioastronomie de Nançay, Observatoire de Paris, Université PSL, CNRS, Univ. Orléans, 18330 Nançay, France


LAM, Pythéas, Aix Marseille Université, CNRS, CNES, 38 Rue Frédéric Joliot Curie, 13013 Marseille, France


DIO, UMS2201 CNRS, Observatoire de Paris, Université PSL, 61 avenue de l’Observatoire, 75014, Paris, France


School of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin, Ireland

Corresponding author: Laurent Lamy,

Received Date: 2021-10-28
Web Publishing Date: 2022-01-13

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 14th 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.

Key words: planetary magnetosphere; Jupiter; auroral radio emissions; planet-moon interaction

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

Laurent Lamy, Baptiste Cecconi, Stéphane Aicardi, C. K. Louis