TY - JOUR
T1 - Tidally Driven Intra-Seasonal Oscillations in the Thermosphere From TIEGCM-ICON and Connections to the Madden-Julian Oscillation
AU - Gasperini, Federico
AU - Maute, Astrid
AU - Wang, Houjun
AU - McClung, Owen
AU - Aggarwal, Deepali
AU - Kumari, Komal
N1 - Publisher Copyright:
© 2025. American Geophysical Union. All Rights Reserved.
PY - 2025/1
Y1 - 2025/1
N2 - Recent evidence has revealed that strong coupling between the lower atmosphere and the thermosphere ((Formula presented.) 100 km) occurs on intra-seasonal (IS) timescales ((Formula presented.) 30–90 days). The Madden-Julian Oscillation (MJO), a key source of IS variability in tropical convection and circulation, influences the generation and propagation of atmospheric tides and is believed to be a significant driver of thermospheric IS oscillations (ISOs). However, limited satellite observations in the “thermospheric gap” (100–300 km) and challenges faced by numerical models in characterizing this region have hindered a comprehensive understanding of this connection. This study uses an Ionospheric Connection Explorer (ICON)-adapted version of the Thermosphere Ionosphere Electrodynamics General Circulation Model, incorporating lower boundary tides from Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) observations, to quantify the impact of the upward-propagating tidal spectrum on thermospheric ISOs and elucidate connections to the MJO. Thermospheric zonal and diurnal mean zonal winds exhibit prominent ((Formula presented.) 20 m/s) tidally driven ISOs throughout 2020–2021, largest at low latitudes (Formula presented.) near 110–150 km altitude. Correlation analyses confirm a robust connection (Formula presented.) between thermospheric ISOs, tides, and the MJO. Additionally, Hovmöller diagrams show eastward tidal propagation consistent with the MJO and concurrent Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) observations. This study demonstrates that vertically propagating tides play a crucial role in linking IS variability from the lower atmosphere to the thermosphere, with the MJO identified as a primary driver of this whole-atmosphere teleconnection. Understanding these connections is vital for advancing our knowledge in space physics, particularly regarding the dynamics of the upper atmosphere and ionosphere.
AB - Recent evidence has revealed that strong coupling between the lower atmosphere and the thermosphere ((Formula presented.) 100 km) occurs on intra-seasonal (IS) timescales ((Formula presented.) 30–90 days). The Madden-Julian Oscillation (MJO), a key source of IS variability in tropical convection and circulation, influences the generation and propagation of atmospheric tides and is believed to be a significant driver of thermospheric IS oscillations (ISOs). However, limited satellite observations in the “thermospheric gap” (100–300 km) and challenges faced by numerical models in characterizing this region have hindered a comprehensive understanding of this connection. This study uses an Ionospheric Connection Explorer (ICON)-adapted version of the Thermosphere Ionosphere Electrodynamics General Circulation Model, incorporating lower boundary tides from Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) observations, to quantify the impact of the upward-propagating tidal spectrum on thermospheric ISOs and elucidate connections to the MJO. Thermospheric zonal and diurnal mean zonal winds exhibit prominent ((Formula presented.) 20 m/s) tidally driven ISOs throughout 2020–2021, largest at low latitudes (Formula presented.) near 110–150 km altitude. Correlation analyses confirm a robust connection (Formula presented.) between thermospheric ISOs, tides, and the MJO. Additionally, Hovmöller diagrams show eastward tidal propagation consistent with the MJO and concurrent Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) observations. This study demonstrates that vertically propagating tides play a crucial role in linking IS variability from the lower atmosphere to the thermosphere, with the MJO identified as a primary driver of this whole-atmosphere teleconnection. Understanding these connections is vital for advancing our knowledge in space physics, particularly regarding the dynamics of the upper atmosphere and ionosphere.
KW - DE3
KW - MJO
KW - TIEGCM-ICON
KW - global-scale waves
KW - intra-seasonal oscillations
KW - ionosphere-thermosphere
UR - https://www.scopus.com/pages/publications/85216000903
U2 - 10.1029/2024JA033178
DO - 10.1029/2024JA033178
M3 - Article
AN - SCOPUS:85216000903
SN - 2169-9380
VL - 130
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 1
M1 - e2024JA033178
ER -