VIP4 takes three inputs: Radial Distance [m], Latitude [rad], and Longitude [rad]. The function performs a spherical harmonic expansion of the magnetic field based on the observations of the Voyager, Pioneer, and IFT probes.
J. E. P. Connerney, M. H. Acuña, N. F. Ness, T. Satoh, "New models of Jupiter's magnetic field constrained by the Io flux tube footprint", Journal of Geophysical Research: Space Physics (1978–2012),
Elias Solorzano (2020). Jupiter's Magnetic Field Model (VIP4) (https://www.mathworks.com/matlabcentral/fileexchange/43852-jupiter-s-magnetic-field-model-vip4), MATLAB Central File Exchange. Retrieved .
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