Model dynamic spectra for the emission of the full auroral oval of an exoplanetary magnetosphere. Abscissa is given in exoplanet’s years (i.e. orbital phase of the exoplanet) and exoplanet’s days (i.e. rotational phase of the exoplanet). In polarization dynamic spectra, black stands for northern emissions, white for southern emissions. a), b) Intensity and polarization dynamic spectra for an axisymmetric planetary magnetic field and 0° inclination (i.e. observer along the orbital plane). c), d) Intensity and polarization dynamic spectra for an axisymmetric planetary magnetic field and 15° inclination (i.e. observer’s direction 15° north of the orbital plane). e), f) Intensity and polarization dynamic spectra for a planetary magnetic field tilted by 15° relative to the rotation axis (perpendicular to the orbital plane) and 0° inclination. g), h) Intensity and polarization dynamic spectra for a planetary magnetic field tilted by 15° and 15° inclination.