Observed Ionospheric Tidal Response to the Madden‐Julian Oscillation

Abstract The Madden‐Julian Oscillation (MJO) is the dominant mode of intraseasonal variability in the tropical troposphere and known to affect the tidal activity in the mesosphere and lower thermosphere (MLT). Using Constellation Observing System for Meteorology, Ionosphere, and Climate‐2 (COSMIC‐2) Global Ionospheric Specification electron density data, we show that the MJO impact extends into the F‐region ionosphere. The MJO imposes an average amplitude variability of 15% in the non‐migrating diurnal tide (DE3) and 2%–5% for the migrating diurnal tide (DW1), with significant responses observed in other diurnal and semidiurnal tidal components. Sounding of the Atmosphere using Broadband Emission Radiometry MLT temperature tides shows no time lag to COSMIC‐2. E‐region dynamo is thus the likely the main mechanism that couples the MJO into the ionosphere. Magnitude and ubiquity of the ionospheric MJO signal underlines the relevance of recurring tropospheric weather patterns for understanding the space weather of the ionosphere.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-09-24
DOI
https://doi.org/10.1029/2025gl115481
Citations
1
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
1.15

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article

Observed Ionospheric Tidal Response to the Madden‐Julian Oscillation

Deepali Aggarwal, Komal Kumari, Jens Oberheide
1 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
1.15
article

Observed Ionospheric Tidal Response to the Madden‐Julian Oscillation

Deepali Aggarwal, Komal Kumari, Jens Oberheide
article en
1 citations

Abstract

Abstract The Madden‐Julian Oscillation (MJO) is the dominant mode of intraseasonal variability in the tropical troposphere and known to affect the tidal activity in the mesosphere and lower thermosphere (MLT). Using Constellation Observing System for Meteorology, Ionosphere, and Climate‐2 (COSMIC‐2) Global Ionospheric Specification electron density data, we show that the MJO impact extends into the F‐region ionosphere. The MJO imposes an average amplitude variability of 15% in the non‐migrating diurnal tide (DE3) and 2%–5% for the migrating diurnal tide (DW1), with significant responses observed in other diurnal and semidiurnal tidal components. Sounding of the Atmosphere using Broadband Emission Radiometry MLT temperature tides shows no time lag to COSMIC‐2. E‐region dynamo is thus the likely the main mechanism that couples the MJO into the ionosphere. Magnitude and ubiquity of the ionospheric MJO signal underlines the relevance of recurring tropospheric weather patterns for understanding the space weather of the ionosphere.

Geophysical Research LettersVol. 52(18)
NSF National Center for Atmospheric Research (US), NSF NCAR High Altitude Observatory (US), Clemson University (US)
National Science Foundation, National Aeronautics and Space Administration, Nuclear Safety and Security Commission
Openalex Percentile: Top 16%
Ionosphere and magnetosphere dynamics
1.15
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