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Tidally Driven Intra-Seasonal Oscillations in the Thermosphere From TIEGCM-ICON and Connections to the Madden-Julian Oscillation

  • Federico Gasperini
  • , Astrid Maute
  • , Houjun Wang
  • , Owen McClung
  • , Deepali Aggarwal
  • , Komal Kumari
  • Orion Space Solutions (OSS), LLC
  • University of Colorado Boulder
  • Clemson University
  • National Center for Atmospheric Research

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

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.

Original languageEnglish
Article numbere2024JA033178
Number of pages25
JournalJournal of Geophysical Research: Space Physics
Volume130
Issue number1
DOIs
StatePublished - Jan 2025

Funding

FG acknowledges support from NSF Grants 2113411 and 2223930; NASA Grants 80NSSC22K0019 and 80NSSC22K1010; and AFOSR Grant FA9550-22-1-0328. ICON is supported by NASA's Explorers Program through contracts NNG12FA45C and NNG12FA42I. AM acknowledges support from NASA ICON award 80NSSC23K1123 and NASA LWS award 80NSSC20K1784.

FundersFunder number
National Science Foundation2113411, 2223930
NSF80NSSC22K0019, 80NSSC22K1010
NASAFA9550-22-1-0328, NNG12FA45C, NNG12FA42I, 80NSSC23K1123, 80NSSC20K1784
AFOSR

    Keywords

    • DE3
    • MJO
    • TIEGCM-ICON
    • global-scale waves
    • intra-seasonal oscillations
    • ionosphere-thermosphere
    • Tiegcm-icon
    • De3
    • Mjo
    • Global-scale waves
    • Intra-seasonal oscillations
    • Ionosphere-thermosphere

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