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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

地球与行星物理（英文）2022，Vol.6Issue(1)：10-12,3.

地球与行星物理（英文）2022，Vol.6Issue(1)：10-12,3.DOI:10.26464/epp2022018

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

Laurent Lamy ¹Baptiste Cecconi ²Stéphane Aicardi ³C.K.Louis¹

作者信息

1. LESIA,Observatoire de Paris,UniversitéPSL,CNRS,Sorbonne Université,Universitéde Paris,5 place Jules Janssen,92195 Meudon,France
2. Station de Radioastronomie de Nan?ay,Observatoire de Paris,UniversitéPSL,CNRS,Univ.Orléans,18330 Nan?ay,France
3. LAM,Pythéas,Aix Marseille Université,CNRS,CNES,38 Rue Frédéric Joliot Curie,13013 Marseille,France
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摘要

关键词

planetary magnetosphere/Jupiter/auroral radio emissions/planet-moon interaction

Key words

planetary magnetosphere/Jupiter/auroral radio emissions/planet-moon interaction

引用本文复制引用

Laurent Lamy,Baptiste Cecconi,Stéphane Aicardi,C.K.Louis..Comment on "Locating the source field lines of Jovian decametric radio emissions" by YuMing Wang et al[J].地球与行星物理（英文）,2022,6(1):10-12,3.

基金项目

We acknowledge the JPL Horizons and IMCCE/MIRIADE ephemer-is services,together with Vratislav Krupar for providing STEREO/Waves high level polarization data.The Jupiter probabil-ity tool at https://jupiter-probability-tool.obspm.fr was developed by the NDA team in the frame of the MASER service supported by the Paris Astronomical Data Centre(PADC)at Observatoire de Par-is.The(unshown)NDA data mentioned in the article are publicly available at https://www.obs-nancay.fr/reseau-decametrique/.We thank the CNES and CNRS/INSU programs of planetology and he-liophysics. （PADC）

地球与行星物理（英文）

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ISSN：2096-3955

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