The data files contain the values of simulated plasma bulk flow velocity components (Vx or Vz) as function of (X, Y, Z) locations in Ganymede-centered GPhiO coordinates, where the X‐axis is along the direction of corotation at the time of Galileo's closest approach to the satellite, the Z‐axis is parallel to the Jovian spin axis and Y completes the right‐handed set (positive toward Jupiter). There are five output files, which correspond to the 5 Galileo close flybys of Ganymede (G2, G7, G8, G28, G29) that are the focus of the analysis of Galileo EPD data by Krupp et al. (2025). Each data file contains columns of the X, Y, Z, Vx or Vz components of the simulated plasma bulk flow velocity.
Krupp, N., E. Roussos, X. Jia, G. Clark, P. Kollmann, K. Khurana, C. Paranicas, A. Galli, M. Franz, S. Barabash, and B. Tsai, Pitch angle distributions of energetic electrons near Ganymede: Galileo EPD measurements, Journal of Geophysical Research – Space Physics, under review.
Text files containing simulated magnetic field vectors in Ganymede-centered spherical (GSPH) coordinates along the trajectories of Galileo and Juno close flybys of Ganymede. Each data file contains columns of the event time (date + hr:min:sec), the radial (Br), polar (Bt) and azimuthal (Bp) components of the simulated magnetic field, except for the G28 flyby output, which contains multiple columns of the simulated magnetic field vectors from simulation time steps of 70 to 131.
Jia, X., M. G. Kivelson, K. K. Khurana, and R. J. Walker (2024), Improved models of Ganymede’s intrinsic and induced magnetic fields based on Galileo and Juno data, Journal of Geophysical Research – Planets, doi:10.1029/2024JE008309, in revision.
