EGU26-2153, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-2153
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 05 May, 10:05–10:15 (CEST)
 
Room 0.94/95
Characteristics of slant sporadic-E layers observed at low-latitudes
Peter T Muka, Marcio TAH Muella, Fredson Conceição-Santos, Laysa CA Resende, Paulo R Fagundes, Olufemi Loius Ogunmola, Pedro Fontes, Valdir Gil Pillat, Mariah Cesar, and Rodolfo de Jesus
Peter T Muka et al.
  • Universidade do Vale do Paraíba, Instituto de Pesquisa e Desenvolvimento, Physics and Astronomy, São José dos Campos - SP, Brazil (ptmuka@univap.br)

This study investigates the occurrence, characteristics, and formation mechanisms of slant sporadic-E layers (Ess). The Ess-type layers observed at the Brazilian low-latitude stations of Jataí (17.9°S, 51.7°W) and São José dos Campos (23.2°S, 45.8°W), are analyzed using ionosonde data recorded for four months (April, June, September, and December) of 2016. Parameters such as top frequency (ftEs), blanketing frequency (fbEs), and virtual height (h’Es) were scaled from ionograms to characterize the slant (Ess) traces. The results show that Ess-type layers predominantly occur at night, forming between 95 and 120 km altitudes, with monthly and local variations. Model simulations using meteor radar-derived winds revealed that strong and stable zonal wind shear are associated with increased Ess-type layer activity. In addition, wavelet spectral analyses of ftEs and fbEs showed that tidal periodicities (diurnal, semidiurnal, terdiurnal, and quarterdiurnal) and their interactions with gravity waves seem to play fundamental roles in the formation of Ess-type layers. A comparison of ΔF (ftEs-fbEs) during Ess-type events confirmed the presence of strong plasma density gradients, supporting the hypothesis that the slanted traces in ionograms result mostly from oblique reflections in inhomogeneous Es layer structures. However, the appearance of slant Es traces may in some cases be related to an actual tilt of the layer. Other relevant aspects of the observations associated with the possible physical mechanisms behind the formation of Ess-type layers at low latitudes are highlighted and discussed

How to cite: Muka, P. T., TAH Muella, M., Conceição-Santos, F., Resende, L. C., Fagundes, P. R., Loius Ogunmola, O., Fontes, P., Gil Pillat, V., Cesar, M., and de Jesus, R.: Characteristics of slant sporadic-E layers observed at low-latitudes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2153, https://doi.org/10.5194/egusphere-egu26-2153, 2026.