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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 31, issue 2
Ann. Geophys., 31, 209–215, 2013
https://doi.org/10.5194/angeo-31-209-2013
© Author(s) 2013. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 31, 209–215, 2013
https://doi.org/10.5194/angeo-31-209-2013
© Author(s) 2013. This work is distributed under
the Creative Commons Attribution 3.0 License.

Regular paper 07 Feb 2013

Regular paper | 07 Feb 2013

The ultra-fast Kelvin waves in the equatorial ionosphere: observations and modeling

A. N. Onohara, I. S. Batista, and H. Takahashi A. N. Onohara et al.
  • Aeronomy Division, Instituto Nacional de Pesquisas Espaciais, São José dos Campos, Brazil

Abstract. The main purpose of this study is to investigate the vertical coupling between the mesosphere and lower thermosphere (MLT) region and the ionosphere through ultra-fast Kelvin (UFK) waves in the equatorial atmosphere. The effect of UFK waves on the ionospheric parameters was estimated using an ionospheric model which calculates electrostatic potential in the E-region and solves coupled electrodynamics of the equatorial ionosphere in the E- and F-regions. The UFK wave was observed in the South American equatorial region during February–March 2005. The MLT wind data obtained by meteor radar at São João do Cariri (7.5° S, 37.5° W) and ionospheric F-layer bottom height (h'F) observed by ionosonde at Fortaleza (3.9° S; 38.4° W) were used in order to calculate the wave characteristics and amplitude of oscillation. The simulation results showed that the combined electrodynamical effect of tides and UFK waves in the MLT region could explain the oscillations observed in the ionospheric parameters.

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