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Influence of the Jovian Current Sheet Models on the Mapping of the UV Auroral Footprints of Io, Europa, and Ganymede
DOI: 10.1029/2023JA032041 Bibcode: 2024JGRA..12932041R

André, N.; Hue, V.; Rabia, J. +4 more

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 widely-used current sheet models, Khurana-2005 (KK2005) and Connerney-2020 (CON2020) combined with the most recent int…

2024 Journal of Geophysical Research (Space Physics)
Ulysses 2
Variation in the Pedersen Conductance Near Jupiter's Main Emission Aurora: Comparison of Hubble Space Telescope and Galileo Measurements
DOI: 10.1029/2023JA032122 Bibcode: 2024JGRA..12932122R

Nichols, J. D.; Vogt, M. F.; Rutala, M. J. +1 more

We present the first large-scale statistical survey of the Jovian main emission (ME) to map auroral properties from their ionospheric locations out into the equatorial plane of the magnetosphere, where they are compared directly to in-situ spacecraft measurements. We use magnetosphere-ionosphere (MI) coupling theory to calculate currents from the …

2024 Journal of Geophysical Research (Space Physics)
Ulysses eHST 2
Stream Interaction Regions in the Minimum of Solar Cycles 23 and 24
DOI: 10.1029/2023JA031685 Bibcode: 2024JGRA..12931685S

Aguilar-Rodriguez, E.; Corona-Romero, P.; Gonzalez-Esparza, J. A. +1 more

Stream interaction regions (SIRs) dominate the large-scale solar wind dynamics during the minimum of the solar cycle. The interaction of SIRs with the magnetosphere causes most of geomagnetic storms during this epoch. We used in-situ solar wind observations at 1 AU to study 62 SIRs detected in the interval 2007-2008 (minimum of cycle 23) and 61 SI…

2024 Journal of Geophysical Research (Space Physics)
Ulysses 1