Abstract
This study develops and validates three photochemical inversion models to retrieve atomic oxygen ion density ([O+]) profiles from 630.0 nm airglow emissions in the mid-latitude ionosphere during geomagnetically quiet period. Using passive ground-based instruments and empirical models, the models were tested and compared against electron density data from FORMOSAT-3/COSMIC (F3/C) and DPS-4 digisonde at Irkutsk. Among the models, Inversion Model 3 showed the strongest agreement with observations, particularly in capturing seasonal variations such as the June–July peak and a secondary March–April peak, which were absent in IRI-2012 predictions. These results highlight the potential of Inversion Model 3 for accurate [O+] retrieval, offering a novel approach for monitoring ionospheric variability using passive photometric observations.
| Original language | English |
|---|---|
| Article number | 55 |
| Journal | Geoscience Letters |
| Volume | 11 |
| Issue number | 1 |
| DOIs | |
| State | Published - Dec 2024 |
Keywords
- 4 digisonde
- Airglow
- COSMIC
- DPS
- Ionosphere F
- Photochemistry
- Region
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