Panels a, b, e, f: examples of Io-controlled jovian radio emissions (of type A, B, C, D, respectively) observed by the NDA. Right-handed (panels a and b) and left-handed (panels e and f) polarization are separated. Panels c, d, g, h: corresponding ExPRES simulated dynamic spectra are computed using the JRM09 model (Connerney et al. 2018), completed by the Connerney et al. (1993) current sheet model, and assuming a source originating from the magnetic field line connected to the main Io Alfvén wing spot on Jupiter and electrons with energies (ϵ_b) of 11 keV (c), 2.5 keV (d), 9 keV (g) and 8 keV (h), respectively.