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• W4300038110 abstract "<strong class=journal-contentHeaderColor>Abstract.</strong> We observed a gravity wave (GW) signature in the OH emission layer in the upper mesosphere, and 4 h later, a medium-scale travelling ionospheric disturbance (MSTID) in the OI 630 nm emission layer. Spectral analysis of the two waves showed that both have almost the same wave characteristics: wavelength, period, phase speed and propagation direction, respectively, 200 km, 60 min, 50 m s<span class=inline-formula>^−1</span>, toward the southeast. From the gravity wave ray-tracing simulation for the mesospheric gravity wave, we found that the wave came from a tropospheric deep convection spot and propagated up to the 140 km altitude. Regarding the same wave characteristics between mesospheric GW and ionospheric MSTID, the two possible cases are investigated: a direct influence of the GW oscillation in the OI 630 nm emission height and the generation of a secondary wave during the GW breaking process. This is the first time to report an observational event of gravity wave propagation from the troposphere, mesosphere to thermosphere–ionosphere in the South American region." @default.
• W4300038110 created "2022-10-03" @default.
• W4300038110 creator A5070125612 @default.
• W4300038110 date "2022-08-10" @default.
• W4300038110 modified "2023-09-30" @default.
• W4300038110 title "Reply on RC2" @default.
• W4300038110 doi "https://doi.org/10.5194/angeo-2022-13-ac4" @default.
• W4300038110 hasPublicationYear "2022" @default.
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