  While lightning activity in Venus is still controversial, its existence in
Jupiter and Saturn was first detected by the Voyager missions and later on
confirmed by Cassini and New Horizons optical recordings in the case of
Jupiter, and recently by Cassini on Saturn in 2009. Based on a recently
developed 3D model we investigate the influence of lightning-emitted
electromagnetic pulses (EMP) on the upper atmosphere of Venus, Saturn and
Jupiter. We explore how different lightning properties such as total energy
released and orientation (vertical, horizontal, oblique) can produce
mesospheric transient optical emissions of different shapes, sizes and
intensities. Moreover, we show that the relatively strong background magnetic
field of Saturn can enhance the lightning-induced quasi-electrostatic and
inductive electric field components above 1000 km of altitude producing
stronger transient optical emissions that could be detected from orbital
probes.
