Abstract
We observed a gravity wave (GW) signature in the OH emission layer in the upper mesosphere, and 4h later, a medium-scale travelling ionospheric disturbance (MSTID) in the OI 630nm 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, 200km, 60min, 50ms-1, 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 140km 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 630nm 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.
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CITATION STYLE
Takahashi, H., Figueiredo, C. A. O. B., Essien, P., Wrasse, C. M., Barros, D., Nyassor, P. K., … Sampaio, A. H. R. (2022). Signature of gravity wave propagations from the troposphere to ionosphere. Annales Geophysicae, 40(6), 665–672. https://doi.org/10.5194/angeo-40-665-2022
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