EGU23-6455
https://doi.org/10.5194/egusphere-egu23-6455
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Planetary-scale MLT waves diagnosed through multi-station methods

Maosheng He
Maosheng He
  • Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China (hmq512@gmail.com)

Most experimental investigations on planetary-scale waves in the mesosphere lower thermosphere (MLT) region are based on single-station or -satellite spectral analysis methods, which are subject to intrinsic spectral aliasing/ambiguity. To conquer the aliasing, the author developed and implemented dual- and multi-station spectral methods in a series of recent works. These methods were implemented on meteor radar observations and surface magnetometer observations. A variety of waves were discovered or investigated in terms of seasonal variations and responses to sudden stratospheric warming events, including lunar and solar tides (migrating and non-migrating), Rossby wave normal modes, quasi-two-day waves, ultra-fast Kelvin waves, and secondary waves of wave-wave nonlinear interactions between the previous waves. The current paper uses synthetic data to illustrate the three methods and reviews comparatively these methods and results in plain language.

How to cite: He, M.: Planetary-scale MLT waves diagnosed through multi-station methods, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-6455, https://doi.org/10.5194/egusphere-egu23-6455, 2023.