Updated Models of Current Sheet and Magnetic Field in the Jovian Magnetosphere for Pre-Galileo, Galileo and Juno Eras

Momoki, Naoya; Toh, Hiroaki

doi:10.1002/essoar.10511021.1

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2022

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“…All the derived data products related to this article are archived in the following repository: https:// repository.kulib.kyoto-u.ac.jp/dspace/handle/2433/276706?locale=en. They were made available by Momoki and Toh (2022).…”

Section: Data Availability Statementmentioning

confidence: 99%

Updated Model Parameters of Current Sheet and Magnetic Field in the Jovian Magnetosphere for Pre‐Galileo, Galileo, and Juno Eras

Momoki

Toh

2022

JGR Planets

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The Jovian magnetosphere has been probed by several spacecraft and thus vector magnetic data have also been accumulated intermittently. Since the first flyby to Jupiter by Pioneer 10 in 1973, six spacecraft (Pioneer 11, Voyager 1, Voyager 2, Ulysses, Cassini, and New Horizons) flew by and five out of them (i.e., except New Horizons) conducted magnetic observations. Galileo (Johnson et al., 1992) was the very first orbiter inserted into Jovicentric orbits, and now Juno (Bolton et al., 2017) is in Jupiter's polar orbits. One of the main applications of the magnetic data is modeling of the Jovian magnetic field, which mainly consists of the Jovian intrinsic and magnetospheric magnetic fields.The Jovian intrinsic field is originated from the dynamo action inside Jupiter. Its models have been studied intensively since the first observation by Pioneer 10, for example,

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Section: Data Availability Statementmentioning

confidence: 99%