Energy dissipation of possible Titan lightning strokes

The search for lightning on Saturnʹs satellite Titan is one scientific target of the Cassini/Huygens mission. Although Voyager 1 did not detect any radio emissions caused by Titan lightning during its flyby in November 1980, one cannot generally rule out their existence, because of low flash rates or ionospheric radiation blockade. Recently, Tokano et al. (Planet. Space Sci. 49 (2001a) 539) have developed a thundercloud model in Titanʹs troposphere favoring the existence of Titan lightning due to negatively charged clouds causing temporary electric fields sufficient to initiate cloud-to-ground lightning strokes. In the present investigation we estimate the amount of energy dissipation of such lightning strokes by electrostatic energy considerations similarly to those by Cooray (J. Geophys. Res. 102(D17) (1997) 21,401). The analysis is based on the cloud charge distribution given by Tokano et al. (2001a), which has a monopole structure or a dipole structure depending on the electrification mechanism. It consists of horizontally homogenous charge layers, whose charge densities depend on the altitude above ground. As results we get the typical charge lowered in a possible Titan lightning stroke and the amount of energy dissipation. For a simulated Titan monopolar cloud charged by electron attachment we found that cloud-to-ground strokes lower about 30 C of charge and dissipate energies about 1010 J. For the modelled bipolar clouds charged by collisional charging these values are a few C of lowered charge and about 108–109J of dissipated energy, which are quite similar to typical Earth values. These energies are substantially higher than the energies suggested by Desch and Kaiser (Nature 343 (1990) 442), who concluded from the Voyager data that discharges might be frequent but weak (<106J). We shortly discuss the detection capability of the Cassini/RPWS (Radio and Plasma Wave Science experiment) for possible Titan lightning strokes taking into account the wave attenuation in the frequency range up to 16 MHz during the propagation through Titanʹs ionosphere as calculated by Schwingenschuh et al. (Adv. Space Res. 28(10) (2001) 1505).