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- W4385994427 abstract "It is well known that lightning occurs frequently within water clouds on Earth (Berger and Vogelsanger in Planet Electrodyn 1:489–510, 1969, Farrell et al. in J Geophys Res Planet 109(E3), 2004; Srinivasan and Gu in 2006 Canadian conference on electrical and computer engineering 2006 May 7, pp 2258–2261. IEEE, 2006). The lightning may also occur within the dust storm or dust devils due to charge transfer by triboelectricity among the dust particles (Farrell et al. in J Geophys Res Planet 109(E3), 2004). The lightning discharge emits low frequency electromagnetic waves along with visible light. The low frequency waves are reflected from the Martian ionosphere and can give rise to Schumann Resonance (SR) in the cavity formed by the Martian surface and the ionosphere. The SR frequency strongly depends on atmospheric conductivity, lightning, the ionospheric turbulence and the surface activity of Mars (Barr et al. in J Atmospher Solar-Terr Phys 62:1689–1718, 2000; Molina-Cuberos et al. J Geophys Res Planets 107:3–1, 2002). There are a few approaches like finite differences (Yang and Pasko in Geophys Res Lett 32(3), 2005), two dimensional telegraph equations (Pechony and Price in Radio Sci 39:1, 2004), full wave equation (Galuk et al. in Telecommun Radio Engin 74(15), 2015) and three dimension Transmission Line Matrix (TLM) method (Toledo-Redondo et al. in Geophys Res Lett 44:648–656, 2017) to study the SR frequency in the planetary atmospheres. The atmosphere of Mars is a non-homogeneous medium, where the low frequency waves can oscillate (Morente et al. in J Geophys Res Space Phys 109(A5), 2004) and the densities are changing with height. In homogeneous atmosphere the gaseous composition is constant with altitude." @default.
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- W4385994427 date "2023-01-01" @default.
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- W4385994427 title "Lightning on Mars" @default.
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