In the terrestrial inner radiation belt, the energy spectrogram of energetic electrons (10-100s keV) sometimes contains one or multiple peaks (Datlowe et al., 1985;Imhof & Smith, 1966;Imhof et al., 1981aImhof et al., , 1981b. These peaks form regular patterns that map on constant bounce-averaged drift frequencies across the entire inner radiation belt (Sauvaud et al., 2013). These features were named "zebra stripes" by Ukhorskiy et al. (2014). Ukhorskiy et al. (2014) first suggested that the stripes are produced by a global process modulating particles' drift motion. Later in Van Allen Probes era, the patterns are observed to be tightening and narrowing during consecutive inner belt crossings (Lejosne & Roederer, 2016;Liu et al., 2016). Liu et al. ( 2016) have shown that a single monochromatic uniform electric field is sufficient for reproducing the key characteristics of the stripes. The authors pointed out that the electric field distorts the electrons' drift shell, so that the electrons detected by the spacecraft at different times are actually originating from different L-shells with different Phase Space Density (PSD). Lejosne and Mozer (2020) further studied the relation of zebra stripes and geomagnetic activity and revealed that zebra stripes are usually triggered during substorm onsets when the penetration electric field is enhanced in the plasmasphere. Similar zebra stripe patterns have been distinguished in Saturn's electron radiation belt (Müller et al., 2010;Paranicas et al., 2007), but only recently it became apparent that their occurrence in the E 100 keV to few MeV range can be explained by global-scale electric fields as at Earth (Hao et al., 2020). Similarly, Hao et al. (2020 attributed this pattern to a convective electric field with an approximate noon-to-midnight orientation and reproduced the stripe patterns seen by Cassini. Indirect evidence in Juno and Galileo data hinted that zebra stripes may also exist at Jupiter but at much higher energies ( E 1 MeV) due to the stronger magnetic field and faster rotation of the planet compared to Saturn and Earth. Noncorotational convection flows at Saturn have long been a candidate among the key sources of the Saturnian electron radiation belt. There are a variety of loss mechanisms in the radiation belt, such as wave-particle scattering into the atmospheric loss cone and electron absorption or energy loss at the Saturnian massive ring system, moons, neutral gas cloud, and dusty rings (