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Planetary Wave Signature in Sporadic E Layer Obtained from Multi-Mission Radio Occultation Observations

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Sobhkhiz-Miandehi,  Sahar
2.3 Geomagnetism, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Jadhav,  Ashish P.

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Arras,  Christina
1.1 Space Geodetic Techniques, 1.0 Geodesy, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Shinagawa,  H.

Miyoshi,  Y.

Yamazaki,  Y.

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5026047.pdf
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Zitation

Sobhkhiz-Miandehi, S., Jadhav, A. P., Arras, C., Shinagawa, H., Miyoshi, Y., Yamazaki, Y. (2024): Planetary Wave Signature in Sporadic E Layer Obtained from Multi-Mission Radio Occultation Observations. - Earth and Space Science, 11, 10, e2024EA003757.
https://doi.org/10.1029/2024ea003757


Zitierlink: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5026047
Zusammenfassung
The Sporadic E layer or Es is an ionospheric phenomenon characterized by enhancements in electron density within 90–120 km above the Earth's surface. Based on the wind shear theory, the formation of Es layers is associated with vertical shears in the horizontal wind, in the presence of the Earth's magnetic field. This study explores the role of planetary waves on inducing these vertical shears and subsequently shaping Es layers. Our investigations benefit from a large amount of data facilitated by the FORMOSAT-7/COSMIC2 and Spire missions, which offer extensive global coverage. A wave analysis is applied to the Es intensity as represented by the S4 index derived from radio occultation measurements, in search of potential planetary wave signatures. Additionally, measurements from Aura/MLS are used to analyze corresponding spectra for the geopotential height, enabling a comparative examination of planetary wave signatures in the Es layer and geopotential height variations. The findings reveal westward and eastward wave components with specific wavenumbers and periods, suggesting the involvement of westward propagating quasi 6-day, quasi 4-day planetary waves, and eastward propagating Kelvin wav