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.
