日本地球惑星科学連合2023年大会

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[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS01] Outer Solar System Exploration Today, and Tomorrow

2023年5月25日(木) 13:45 〜 15:00 106 (幕張メッセ国際会議場)

コンビーナ:木村 淳(大阪大学)、佐柳 邦男 M(NASA Langley Research Center)、土屋 史紀(東北大学大学院理学研究科惑星プラズマ・大気研究センター)、座長:佐柳 邦男(NASA Langley Research Center)、木村 淳(大阪大学)

14:15 〜 14:30

[PPS01-13] Jovian auroral radio source occultation modelling and application to the JUICE science mission planning

*Baptiste Cecconi1、Corentin K Louis2、Claudio Muñoz Crego3、Claire Vallat4 (1.LESIA, Observatoire de Paris, CNRS, PSL Research University、2.School of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin, Ireland、3.Aurora B.V., for European Space Agency, ESAC, Madrid, Spain、4.Rhea Group, for European Space Agency, ESAC, Madrid, Spain)

キーワード:Planetary radio emissions, Jupiter, Modeling

Occultations of the Jovian low frequency radio emissions by the Galilean moons have been observed by the PWS (Plasma Wave Science) instrument of the Galileo spacecraft. We show that the ExPRES (Exoplanetary and Planetary Radio Emission Simulator) code accurately models the temporal occurrence of the occultations in the whole spectral range observed by Galileo/PWS. This validates of the ExPRES code. In addition to supporting the analysis of the science observations, the method can be applied for preparing the JUICE moon flyby science operation planning.