EGU26-15839, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-15839
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, X4.133
Formation and evolution of nighttime MSTID modulated by the atmospheric tides
Longchang Sun1, Jiyao Xu2, Weiyuan Yuan3, and Yajun Zhu4
Longchang Sun et al.
  • 1National Space Science Center of Chinese Academy of Sciences, China (sunlongchang@nssc.ac.cn)
  • 2National Space Science Center of Chinese Academy of Sciences, China (xujiyao@nssc.ac.cn)
  • 3National Space Science Center of Chinese Academy of Sciences, China (yuanwei@nssc.ac.cn)
  • 4National Space Science Center of Chinese Academy of Sciences, China (y.zhu@swl.ac.cn)

In this report, we utilize data from the multi-ground-based instruments of the Chinese Meridian Project (CMP) and public national websites, including red-line all-sky airglow imagers, digisondes, GNSS-TEC receivers, and so on, to conduct an in-depth investigation into the formation and evolution processes as well as the accompanying physical mechanisms of two nighttime MSTID events occurring over the mid- and low-latitude regions of China. Specifically, we focus on the impacts of the hourly tidal-induced atmospheric dynamo process and its modulation effect on ionospheric electron density (airglow), which in turn affect the formation and evolution of these nighttime MSTIDs. The specific physical processes associated with the nighttime MSTIDs are discussed.

How to cite: Sun, L., Xu, J., Yuan, W., and Zhu, Y.: Formation and evolution of nighttime MSTID modulated by the atmospheric tides, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15839, https://doi.org/10.5194/egusphere-egu26-15839, 2026.