EGU24-2764, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-2764
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Observed responses of tides and gravity waves in the MLT region to the Madden-Julian Oscillation

Xu Zhou1,2,3, Xinan Yue1,2,3, Libo Liu1,2,4, Guiwan Chen5, Xian Lu6, You Yu1,2,3, and Lianhuan Hu1,3
Xu Zhou et al.
  • 1Institute of Geology and Geophysics, Chinese Academy of Sciences, Key Laboratory of Earth and Planetary Physics, China (zx0601@mail.iggcas.ac.cn)
  • 2College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, China
  • 3Beijing National Observatory of Space Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, China
  • 4Heilongjiang Mohe National Geophysical Observatory, Institute of Geology and Geophysics, Chinese Academy of Sciences, China
  • 5State Key Laboratory of Numerical Modeling for Atmospheric Sciences and Geophysical Fluid Dynamics, Institute of Atmospheric Physics, Chinese Academy of Sciences, China
  • 6Department of Physics and Astronomy, Clemson University, Clemson, USA

This work analyzed the intraseasonal variability of non-migrating tides DE3 and gravity wave momentum fluxes (GWMF) in the mesosphere and lower thermosphere (MLT) region and discussed the possible connection with the tropospheric MJO. Based on the joint observations of the TIMED-TIDI satellite and the 120°E meridian meteor radar chain, we revealed a significant broad-band intra-seasonal signal in the DE3 amplitude around the equator with a clear seasonal dependence. The intraseasonal variability of DE3 in zonal winds (DE3-U) has a strong amplitude in boreal winter, up to 1-2 times the seasonal average, while the variability is usually within 20% during other seasons. The response of MLT DE3 tides to the MJO in different seasons was further discussed together with the MJO activity index. The results suggested that the DE3-U in boreal winter generally has a larger amplitude during MJO phases 4–6 (~10%–40%), while the amplitude is smaller for other MJO phases (~−10%–−40%). As for the GWMF estimation, the 12-year continuous observation of the Mohe meteor radar (53.5°N, 122.3°E) was analyzed. The results showed that intraseasonal GWMF variability is also prominent during boreal winter. Composite analysis for DJF season according to MJO phases revealed that the zonal GMWFs notably increased in MJO P4 by ~2–4 m2/s2, and a Monte Carlo test was designed to examine the statistical significance. The response in zonal winds differs from the GMWF response by two MJO phases (i.e., 1/2π). Additionally, time-lagged composites revealed the strengthened westward GWMF occurred ~25–35 days after MJO P4, coincident with the MJO impact on the polar vortex as previous works revealed. Overall, this work emphasized that the tropical sources (MJO) impress the intraseasonal signal from the troposphere to the MLT region, either tropics or extratropics.

How to cite: Zhou, X., Yue, X., Liu, L., Chen, G., Lu, X., Yu, Y., and Hu, L.: Observed responses of tides and gravity waves in the MLT region to the Madden-Julian Oscillation, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-2764, https://doi.org/10.5194/egusphere-egu24-2764, 2024.