EGU25-3631, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-3631
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 14:00–15:45 (CEST), Display time Thursday, 01 May, 14:00–18:00
 
Hall X4, X4.168
Estimation of the energy of Jovian lightning discharges based on the analysis of rapid whistlers detected by Juno
Katerina Rosicka1,2, Ondřej Santolík1,2, Ivana Kolmašová1,2, Masafumi Imai1, and William Kurth3
Katerina Rosicka et al.
  • 1Institute of Atmospheric Physics, Czech Academy of Science, Prague, Czechia
  • 2Faculty of Mathematics and Physics, Charles University, Prague, Czechia
  • 3University of Iowa, Iowa City, USA

Jupiter was the first planet other than Earth, where lightning discharges were detected using the radio wave measurements of the Voyager spacecraft in 1979. Starting with Voyager 1, all spacecraft missions to Jupiter detected lightning as bright spots in the optical images of the nightside of the planet. The Juno spacecraft currently orbits Jupiter and its measurements in the audible frequency range below 20 kHz often show rapid whistlers, electromagnetic signatures of electrical discharges with very low dispersion. These measurements represent the largest known database of lightning detections at this planet.

We explore the Juno measurements of rapid whistlers in order to estimate their amplitudes which, in turn, can help us to estimate the energy radiated in this part of the electromagnetic spectrum from the Jovian lightning discharges. We use a newly developed method based on the search for sufficiently large coherent structures in the spectrograms of rapid whistlers. The choice of the parameters of this method is supported by extensive modeling to ensure that the probability of false positive detections is reasonably low. Another set of simulations is performed for different backgrounds to estimate the minimum detectable amplitude of the rapid whistlers.

In total, our analysis includes 1357 rapid whistlers from the first 8 perijoves, and we take into account a geometrical correction based on changing attitude of the spacecraft and its varying distance from the top of the ionosphere (300-km altitude above the 1-bar level). After performing these normalizations, we estimate the energy which was radiated from the source lightning discharges into the rapid whistlers. We obtain a wide distribution of values with a range of 308–3341 J between the lower and upper quartiles, and with the median value of 973 J. These energies are similar to energies of electromagnetic waves radiated at audible frequencies from the terrestrial lightning discharges. Our result differs from most of the previous estimates of lightning energies at Jupiter, which found them much larger than at Earth. However, our results are consistent with the latest optical measurements onboard Juno.

How to cite: Rosicka, K., Santolík, O., Kolmašová, I., Imai, M., and Kurth, W.: Estimation of the energy of Jovian lightning discharges based on the analysis of rapid whistlers detected by Juno, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3631, https://doi.org/10.5194/egusphere-egu25-3631, 2025.