Abstract: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 3‐D model, we investigate the influence of lightning‐emitted electromagnetic pulses on the upper atmosphere of Venus, Saturn, and Jupiter. We explore how different lightning properties such as total energy relea… Show more
“…(2014) estimated that for Jupiter the peak photon density for elves would be at an altitude of 250–300 km, and Pérez‐Invernón et al. (2017) found that the width of elves in Jupiter's atmosphere could be between ∼400 km for horizontal discharge and ∼800 km for vertical discharge. For both sprites and elves, the characteristic decay times can vary from submillisecond to several milliseconds, depending on the parameters used in the model (Dubrovin et al., 2014; Luque et al., 2014).…”
• Eleven transient bright flashes were observed by the ultraviolet instrument on the Juno mission • The flashes have an average duration of 1.4 ms, are located 260 km above the 1-bar level and are dominated by H 2 emission • The observations are consistent with transient luminous events which occur in the upper atmosphere in response to tropospheric lightning
“…(2014) estimated that for Jupiter the peak photon density for elves would be at an altitude of 250–300 km, and Pérez‐Invernón et al. (2017) found that the width of elves in Jupiter's atmosphere could be between ∼400 km for horizontal discharge and ∼800 km for vertical discharge. For both sprites and elves, the characteristic decay times can vary from submillisecond to several milliseconds, depending on the parameters used in the model (Dubrovin et al., 2014; Luque et al., 2014).…”
• Eleven transient bright flashes were observed by the ultraviolet instrument on the Juno mission • The flashes have an average duration of 1.4 ms, are located 260 km above the 1-bar level and are dominated by H 2 emission • The observations are consistent with transient luminous events which occur in the upper atmosphere in response to tropospheric lightning
“…Possible extrasolar lightning tracer are chemical species like HCN and C2H (Rimmer & Helling 2016;Hodosán et al 2016b;Ardaseva et al 2017), or spectral peculiarities like lightning modulated coherent cyclotron emission coming from electrons that are accelerated by the planet's magnetic field (Vorgul & Helling 2016;Helling & Vorgul 2017) similar to the lightning modulated cosmic ray air showers recently discovered on Earth (Schellart et al 2015;Trinh et al 2017). Moreover, strong large-scale magnetic fields like on Saturn (or Brown Dwarfs) enhance lightning-induced electric fields producing strong transient optical emission as demonstrated for Earth (Pérez-Invernón et al 2017). As lightning requires the presence of clouds, lightning indicators are formidable tool to prove the presence of clouds in exoplanet atmosphere as well as gaining insight into the atmospheric dynamics.…”
Section: Lightning On Exoplanet and The Extrasolar Global Electric Ci...mentioning
Clouds also form in atmospheres of planets that orbit other stars than our Sun, in so-called extrasolar planets or exoplanets. Exoplanet atmospheres can be chemically extremely rich. Exoplanet clouds are therefor made of a mix of materials that changes throughout the atmosphere. They affect the atmospheres through element depletion and through absorption and scattering, hence, they have a profound impact on the atmosphere's energy budget. While astronomical observations point us to the presence of extrasolar clouds and make first suggestions on particle sizes and material compositions, we require fundamental and complex modelling work to merge the individual observations into a coherent picture. Part of this is to develop an understanding for cloud formation in non-terrestrial environments.
“…As in the model of halos, we can choose the characteristics of the lightning discharge that produces the elve. The details of this elve model can be found in Inan et al (), Taranenko et al (), Kuo et al (), Marshall et al (), Inan and Marshall (), Luque et al (), Marshall et al (), Pérez‐Invernón et al (), Liu et al (), and Pérez‐Invernón et al ().…”
In this work, we develop two spectroscopic diagnostic methods to derive the peak reduced electric field in transient luminous events (TLEs) from their optical signals. These methods could be used to analyze the optical signature of TLEs reported by spacecraft such as Atmosphere‐Space Interactions Monitor (European Space Agency) and the future Tool for the Analysis of RAdiations from lightNIngs and Sprites (Centre National d'Études Spatiales). As a first validation of these methods, we apply them to the predicted (synthetic) optical signatures of halos and elves, two types of TLEs, obtained from electrodynamical models. This procedure allows us to compare the inferred value of the peak reduced electric field with the value computed by halo and elve models. Afterward, we apply both methods to the analysis of optical signatures of elves and halos reported by Global LIghtning and sprite MeasurementS (Japan Aerospace Exploration Agency) and Imager of Sprites and Upper Atmospheric Lightning (National Space Organization) spacecraft, respectively. We conclude that the best emission ratios to estimate the maximum reduced electric field in halos and elves are the ratio of the second positive system of N2 to first negative system (FNS) of N
2+, the first positive system of N2 to FNS of N
2+ and the Lyman‐Birge‐Hopfield band of N2 to FNS of N
2+. In the case of reduced electric fields below 150 Td, we found that the ratio of the second positive system of N2 to first positive system of N2 can also be used to reasonably estimate the value of the field. Finally, we show that the reported optical signals from elves can be treated following an inversion method in order to estimate some of the characteristics of the parent lightning.
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