This dataset contains model results from a magnetohydrodynamic (MHD) model of Ganymede's magnetosphere adapted to Juno's PJ34 flyby in 2021. Here we publish coordinates for the predicted location of the open-closed-field line-boundary (OCFB) on Ganymede's surface. Additionally we provide coordinates of Juno's magnetic footprint, namely the surface locations that connect to Juno's trajectory through magnetic field lines. For the surface locations we use a western longitude planetographic coordinate system where 0° longitude is in direction of the y-axis and 90° in direction of the x-axis of the cartesian GPhiO system. The GPhiO system is defined by the primary direction z parallel to Jupiter’s rotation axis, the secondary direction y is poi...
[1] Ganymede is unique among planetary moons because it has its own magnetic field strong enough to ...
Data repository for the study entitled "Modeling of Ganymede's Magnetic and Plasma Environment Durin...
The Galilean satellite auroral footprints result from the interaction between the co-rotating iogeni...
This dataset contains model results from a magnetohydrodynamic (MHD) model of Ganymede's magnetosphe...
On 7 June 2021 the Juno spacecraft visited Ganymede and provided the first in situ observations sinc...
This dataset contains model results from a magnetohydrodynamic (MHD) model of Ganymede's magnetosphe...
International audienceJuno's flyby of Ganymede on 7 June 2021, provides a unique opportunity to expl...
The submitted work describes a study of the auroral footprints triggered by the Galilean moons Europ...
The Juno spacecraft has been in orbit around Jupiter since 2016. Two flybys of Ganymede were execute...
This dataset provides the modeling results for the paper 'Driver of Energetic Electron Precipitation...
This thesis reports on studies of magnetic field observations obtained by the NASA Juno spacecraft c...
On 7 June 2021, NASA's Juno mission obtained unique measurements of Ganymede's magnetosphere during ...
peer reviewedJupiter's satellite auroral footprints are a manifestation of the satellite-magnetosphe...
We present here a study of the latitudinal variations of the location of Ganymede’s footprint (GFP) ...
A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic field o...
[1] Ganymede is unique among planetary moons because it has its own magnetic field strong enough to ...
Data repository for the study entitled "Modeling of Ganymede's Magnetic and Plasma Environment Durin...
The Galilean satellite auroral footprints result from the interaction between the co-rotating iogeni...
This dataset contains model results from a magnetohydrodynamic (MHD) model of Ganymede's magnetosphe...
On 7 June 2021 the Juno spacecraft visited Ganymede and provided the first in situ observations sinc...
This dataset contains model results from a magnetohydrodynamic (MHD) model of Ganymede's magnetosphe...
International audienceJuno's flyby of Ganymede on 7 June 2021, provides a unique opportunity to expl...
The submitted work describes a study of the auroral footprints triggered by the Galilean moons Europ...
The Juno spacecraft has been in orbit around Jupiter since 2016. Two flybys of Ganymede were execute...
This dataset provides the modeling results for the paper 'Driver of Energetic Electron Precipitation...
This thesis reports on studies of magnetic field observations obtained by the NASA Juno spacecraft c...
On 7 June 2021, NASA's Juno mission obtained unique measurements of Ganymede's magnetosphere during ...
peer reviewedJupiter's satellite auroral footprints are a manifestation of the satellite-magnetosphe...
We present here a study of the latitudinal variations of the location of Ganymede’s footprint (GFP) ...
A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic field o...
[1] Ganymede is unique among planetary moons because it has its own magnetic field strong enough to ...
Data repository for the study entitled "Modeling of Ganymede's Magnetic and Plasma Environment Durin...
The Galilean satellite auroral footprints result from the interaction between the co-rotating iogeni...