the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Spectroscopic detection of terrestrial lightning from space by JUICE-MAJIS during Earth Gravity Assist
Abstract. A lightning event was detected by the MAJIS imaging spectrometer onboard the Jupiter Icy Moons Explorer (JUICE) spacecraft during its first Earth gravity assist maneuver. This serendipitous space-based spectroscopic observation represents the first detection of its kind for any planetary atmosphere. The event, composed of four flashes, was registered on 2024, August, 20th in an area offshore of Sumatra island, during local nighttime, near to optically thick clouds probed by MAJIS thermal wavelengths. No coincident detection has been obtained by ground-based lightning sensor networks, yet MAJIS observations provide unambiguous evidence of neutral atomic oxygen and nitrogen emissions, identified through several diagnostic lines. A faint Hα signature may also tentatively be associated with lightning flashes.
As MAJIS is not optimized for such observations, a number of caveats related to spectral and temporal resolutions have been considered when deriving absolute quantities, such as lightning energy and temperature. Retrieved energies are overall consistent with known emission by lightning of average strength, ranging from (0.7 ± 0.2) to (1.3 ± 0.3) MJ in the 777 nm O I line and from (0.5 ± 0.2) to (1.5 ± 0.4) MJ in the 870 nm N I line. Temperature estimates, more sensitive to observing biases, yield a broad range of values, spanning between 5000 and 20000 K, with standard uncertainties of the order of 2000–3000 K depending on the retrieval method.
This observation represents a useful benchmark for guiding detection and interpreting possible lightning events on Jupiter, a primary target of the JUICE mission. A preliminary extrapolation of the terrestrial case to the conditions of Jovian atmosphere suggests that H I emissions in the 650 nm and 1870 nm spectral ranges are the most promising for identifying lightning on Jupiter with the MAJIS instrument.
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Status: open (until 26 Mar 2026)
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RC1: 'Comment on egusphere-2025-6453', Anonymous Referee #1, 23 Feb 2026
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AC1: 'Reply on RC1', Emiliano D'Aversa, 25 Feb 2026
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[radio obs and synergies]
- Both historical and more recent radio and microwave measurements at Jupiter (and other planets) are recalled at the beginning of Section 4.6. Regarding future JUICE detections, we agree with the reviewer that synergistic observations will add value to lightning studies. Anyway, as already pointed out by the reviewer, a more in-depth discussion seems off-topic in this context, since we are only preliminary discussing how MAJIS might detect lightning on Jupiter. It is also worth noting that the probability of a coincident detection, e.g. by MAJIS and RPWI, of the same lightning event is reduced by the strict constraints on both spacecraft position and MAJIS pointing/timing. Conversely, general synergy in global statistical analyses could be more easily envisaged.
- We take advantage of this point raised to add a brief comment about synergies at the very end of the conclusion (Section 5) ("In that case, several synergistic approaches with other JUICE instruments can be envisaged, like with UVS for detecting shorter-wavelength emission lines, with JANUS for higher spatial resolution and context images, or with RPWI for coincident radio signals. Even if the likelihood of simultaneous observations of the same event will decrease proportionally to the number of observing constraints to be satisfied, a comparison of events on a statistical basis at global scale could be achieved.")
[observation timing]
- We confirm that the MAJIS time sequence contains long gaps among acquisitions: obs[22ms],gap[178ms],obs[22ms],gap[178ms],etc... and that this was done in order to avoid spatial gaps on the surface, given the high flyby speed. The temporal issue of the observations arises from the fact that we cannot know what was the temporal variability of the lightning flashes, what number of strokes they were made of, their lifetime and exact timing. This is why we could only derive the integrated energy as a lower limit (only that registered during acquisitions, not gaps) and we have large discrepancies in temperature retrievals. We will add a further comment in Section 3.5 to make this point clearer ("A further source of uncertainty is the presence of large temporal gaps between MAJIS acquisitions: consecutive frames start 200 ms apart but the signal is integrated for only 22 ms, leaving 178 ms gaps between them. Therefore, we have no information not only on the number of strokes occurring but also whether the detectable flashes were shorter or longer than 22 ms, and which portion of their lifetime is sampled by the MAJIS acquisitions or falls within the gaps.")
- The only further quantitative estimate we could make concerns the integrated energy: if we assume the average energy measured in flashes B,C,D to be also emitted during the gaps between B-C and C-D, the final total energy increases by a factor (22x3+200x2)/(22x3) ~ 7.1. However, we deem this to be a rather arbitrary assumption, since we do not know which portions of flash light curves fall inside the acquisition intervals and which ones in the gaps in between. Therefore, to avoid making the results more confusing, we would prefer to keep only the lower limit indicated.
- To this regard, we add in Section 4.2 a citation of the work by Wemhoner et al.2025, where they compare lightning energy derived from ground- and space-based observations (their fig.6c) ("As highlighted by systematic comparisons of ground- and space-based lightning observations, the energy measured from space can be significantly lower than that from ground, probably due to the fact that most of the optical energy emitted by a return stroke comes from its near-ground portion, thus considerably absorbed by overlying clouds (Wemhoner et al.2025).")
["kelvin" --> "Kelvin"]
- No problem in changing it, even if, in the usage as measurement unit, the lowercase should be more appropriate (e.g. https://chec.engineering.cornell.edu/units-of-measurement/). We leave it to the editor's choice.
[further references]
- We are very grateful to the reviewer for highlighting interesting references that we have not covered.
- A citation of Kákona et al.(2023) will be added in discussing temporal issues (Section 3.5);
- Wemhoner et al.(2026) retrieve 17600 K as average peak temperatures for CG flashes, in line with our large retrieved range (citation to be added in Section 4.3.3).
Citation: https://doi.org/10.5194/egusphere-2025-6453-AC1
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AC1: 'Reply on RC1', Emiliano D'Aversa, 25 Feb 2026
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Review of egusphere-2025-6453
Spectroscopic detection of terrestrial lightning from space by JUICE-MAJIS during Earth Gravity Assist
by Emiliano d’Aversa et al.
The authors convincingly argue that terrestrial lightning has benn spectroscopically observed with the JUICE-MAJIS instrument during the Earth Gravity Assist flyby. The analysis is quantitative, detailed and covers multiple aspects. Discussed is both the observation of terrestrial lightning as well as an outlook on future observations at Jupiter. Not mentioned are the effects of lightning in the radio spectrum, prominently VLF whistlers. These have been observed historically and numerously, on the ground and also in space. JUICE has also the RPW (radio and plasma waves), this could enable coordinated optical and radio waves analysis and studies of lightning. However, this can be left for the future. The manuscript is already quite rich. I recommend to publish the work after only minor comments.
Minor comments:
Lines 153-156: "It has been obtained by rotating the line of sight by about 4° (2° of rotation of the internal mirror) in steps for a total time of seconds. At every step (i.e. every 200 ms), a 128-pixels spectral frame encompassing 1016 wavelengths has been acquired, with an integration time of 22 ms." This is a bit confusing for me: Does it mean, that there are gaps in time, in a 200 ms long step the integration happens for 22 ms, i.e. about 11% of the time. At the other time (~89%) no integration of light is going on? I understand that the motion of the mirror is adjusted to the distance to the planet/moon (11500 km at EGA) and spacecraft rotation such that there spatial gaps are avoided: pixel width on Earth ~1.7 km (2 km with motional smearing). The duration of lightning flashes measured on the ground varies, a median duration of 0.52 s is given in Kákona et al., 2023, so the 200 ms step duration would be no problem, However, a flash typically consists of much shorter "strokea". This temporal characteristics of lightning flashes is discussed in section 3.5, but the possible effects of the integration in time by MAIJIs with gaps (if I understood correctly) and of relatively slow sampling (200 ms) could perhaps be elaborated on a bit more.
Line 301: "kelvin" --> "Kelvin"
Section 3.3 Oxygen lines
A recent publication with temperature estimates in lightning based on atomic oxygen lines (observed at the ground) is by Wemhoner et al. (2026). I'm not sure how relevant this would be for the discussion in this manuscript, and suggest to the authors to have a look at this paper.
Section 3.5. Temporal resolution
Kákona et al. (2023), already mentioned above, might be a fresh reference with some relevance for this discussion.
References
Kákona, J., Mikeš, J., Ambrožová, I., Ploc, O., Velychko, O., Sihver, L., and Kákona, M.: In situ ground-based mobile measurement of lightning events above central Europe, Atmos. Meas. Tech., 16, 547–561, https://doi.org/10.5194/amt-16-547-2023, 2023.
Wemhoner, J., Leal, A.F.R., da Silva, C.L. et al. Atomic oxygen photometric temperature of lightning and its sub-processes with SOPAPILLA. Sci Rep 16, 4068 (2026). https://doi.org/10.1038/s41598-025-34189-8