EGU26-16559, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-16559
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 06 May, 10:45–12:30 (CEST), Display time Wednesday, 06 May, 08:30–12:30
 
Hall X4, X4.132
Short-Term Tidal Modal Variability in the MLT Revealed by Combined ICON/MIGHTI and Meteor Radar Chain Observations
Han Ma1, Maosheng He1, Xu Zhou2, and Libo Liu2
Han Ma et al.
  • 1National Space Science Center, Chinese Academy of Sciences
  • 2Institute of Geology and Geophysics, Chinese Academy of Sciences

Atmospheric tides propagating upward from the lower atmosphere undergo nonlinear interactions and modulate ionospheric plasma redistribution, leading to pronounced day-to-day variability in ionospheric parameters. This variability reflects the superposition of multiple tidal components with different periods, zonal wavenumbers, and mode structures, yet the dominant modes remain unclear. A hybrid method that combines space-based observations (ICON/MIGHTI), ground-based measurements (Chinese meteor radar chain), and empirical tidal modes (ETMs) is applied to extract the short-term tidal variability. The method is validated during the 2021 sudden stratospheric warming event, capturing the enhancement of the SW2 tidal amplitude, a strengthened first antisymmetric mode, and the phase advance in E-region neutral winds. Future work will extend this approach to assess the modal contributions of tides to the variability of ionospheric plasma drift.

How to cite: Ma, H., He, M., Zhou, X., and Liu, L.: Short-Term Tidal Modal Variability in the MLT Revealed by Combined ICON/MIGHTI and Meteor Radar Chain Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16559, https://doi.org/10.5194/egusphere-egu26-16559, 2026.