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相关论文: Ganymede MHD Model: Magnetospheric Context for Jun…

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We report on dust measurements obtained during the seventh orbit of the Galileo spacecraft about Jupiter. %which had a close flyby at Ganymede. The most prominent features observed are highly time variable dust streams recorded throughout…

天体物理学 · 物理学 2015-06-24 H. Krüger , E. Grün , A. Graps , A. Heck , S. Lammers

We report results of Hubble Space Telescope observations from Ganymede's orbitally trailing side which were taken around the flyby of the Juno spacecraft on June 7, 2021. We find that Ganymede's northern and southern auroral ovals alternate…

An empirical formula recently appeared in the literature to explain the observed anomalies of about $\Delta\dot\rho\approx 1-10$ mm s$^{-1}$ in the geocentric range-rates $\dot\rho$ of the Galileo, NEAR and Rosetta spacecraft at some of…

广义相对论与量子宇宙学 · 物理学 2014-11-10 Lorenzo Iorio

Ganymede's aurora are the product of complex interactions between its intrinsic magnetosphere and the surrounding Jovian plasma environment and can be used to derive both atmospheric composition and density. In this study, we analyzed a…

地球与行星天体物理 · 物理学 2024-09-12 Zachariah Milby , Katherine de Kleer , Carl Schmidt , François Leblanc

In this paper, we model the plasma environment of Ganymede by means of a collisionless test particle simulation. By coupling the outputs from a DSMC simulation of Ganymede's exosphere (i.e. number density profiles of neutral species such as…

地球与行星天体物理 · 物理学 2025-02-19 Arnaud Beth , Marina Galand , Ronan Modolo , Xianzhe Jia , François Leblanc , Hans Huybrighs

The in-situ characterization of moon-magnetosphere interactions at Jupiter and the mapping of moon auroral footpaths require accurate global models of the magnetospheric magnetic field. In this study, we compare the ability of two…

地球与行星天体物理 · 物理学 2024-01-19 Jonas Rabia , Quentin Nénon , Nicolas André , Vincent Hue , Daniel Santos-Costa , Aneesah Kamran , Michel Blanc

The interaction between Jupiter's magnetosphere and the solar wind is not well-constrained: while internal energetic plasma processes are thought to dominate plasma circulation, the solar wind nonetheless exerts significant control over the…

In the last decades there have been an increasing interest in improving the accuracy of spacecraft navigation and trajectory data. In the course of this plan some anomalies have been found that cannot, in principle, be explained in the…

地球与行星天体物理 · 物理学 2018-05-02 L. Acedo , P. Piqueras , J. A. Moraño

Spacecraft data reveal a very Earth-like Jovian magnetic field. This is surprising since numerical simulations have shown that the vastly different interiors of terrestrial and gas planets can strongly affect the internal dynamo process.…

地球与行星天体物理 · 物理学 2015-06-22 T. Gastine , J. Wicht , L. Duarte , M. Heimpel , A. Becker

Jupiter's internal flow structure is still not fully known, but can be now better constrained due to Juno's high-precision measurements. The recently published gravity and magnetic field measurements have led to new information regarding…

地球与行星天体物理 · 物理学 2019-07-17 Keren Duer , Eli Galanti , Yohai Kaspi

During its 53-day polar orbit around Jupiter, Juno often crosses the boundaries of the Jovian magnetosphere (namely the magnetopause and bow shock). From the boundary locations, the upstream solar wind dynamic pressure can be inferred,…

The abrupt boundary between a magnetosphere and the surrounding plasma, the magnetopause, has long been known to support surface waves. It was proposed that impulses acting on the boundary might lead to a trapping of these waves on the…

空间物理 · 物理学 2019-02-13 M. O. Archer , H. Hietala , M. D. Hartinger , F. Plaschke , V. Angelopoulos

The new data delivered by NASA's Juno spacecraft significantly increase our understanding of Jupiter's internal dynamics. The gravity data constrain the depth of the zonal flows observed at cloud level and suggest that they slow down…

地球与行星天体物理 · 物理学 2023-06-07 Johannes Wicht , Thomas Gastine , Lucia D. V. Duarte , Wieland Dietrich

The Juno mission will measure Jupiter's magnetic field with unprecedented precision and provide a wealth of additional data that will allow to constrain the planet's interior structure and dynamics. Here we analyse 66 numerical simulations…

地球与行星天体物理 · 物理学 2017-09-13 Lucia D. V. Duarte , Johannes Wicht , Thomas Gastine

Magnetic sounding using data collected from the Juno mission can be used to provide constraints on Jupiter's interior. However, inwards continuation of reconstructions assuming zero electrical conductivity and a representation in spherical…

地球与行星天体物理 · 物理学 2024-05-06 Philip W. Livermore , Leyuan Wu , Longwei Chen , Sjoerd A. L. de Ridder

The JUNO mission to Jupiter is planned to measure the water abundance in Jupiter's atmosphere below the cloud layer. This measurement is important because it can be used to reveal valuable information on Jupiter's origin and its…

地球与行星天体物理 · 物理学 2015-06-19 Ravit Helled , Jonathan Lunine

We investigate the magnetic signature of oceanic circulation in Ganymede's subsurface ocean using kinematic induction modeling. Our approach couples zonal jet flows from rotating thermal convection simulations with magnetic field models…

地球与行星天体物理 · 物理学 2026-03-09 Simon Cabanes , Thomas Gastine , Alexandre Fournier

During Juno's only flyby of Europa, the Jupiter Energetic Particle Detector Instrument (JEDI) measured complex dropouts in the energetic ion flux in Europa's wake. We investigate the causes of these dropouts, focusing specifically on…

Deciphering the flow below the cloud-level of Jupiter remains a critical milestone in understanding Jupiter's internal structure and dynamics. The expected high-precision Juno measurements of both the gravity field and the magnetic field…

地球与行星天体物理 · 物理学 2019-02-13 Eli Galanti , Hao Cao , Yohai Kaspi

Gravity assist manoeuvres are one of the most succesful techniques in astrodynamics. In these trajectories the spacecraft comes very close to the surface of the Earth, or other Solar system planets or moons, and, as a consequence, it…

空间物理 · 物理学 2017-01-25 L. Acedo
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