Direct Observations of Large‐Scale Wave Structure and Post‐Sunset Rise of the Ionosphere in the Generation of Equatorial Spread F
Year: 2026
Type: article
Abstract: Large‐scale wave structure (LSWS) and the post‐sunset rise (PSSR) are two key factors in the generation of equatorial spread F (ESF). In this study, we reported continuous and direct observations of LSWS and PSSR and their effects on seeding ESF by Sanya incoherent scatter radar (SYISR) and ionosonde in September–October 2024. SYISR data indicated distinct day‐to‐day variability in LSWS, characterized by variable zonal wavelengths and periods with mean values of 436 km and 52 min, respectively. Ray‐tracing simulations demonstrated that the upwelling and propagation of LSWS greatly affect signature features of frequency range and virtual height of satellite traces in ionograms. Further analysis revealed that ESF occurrence rate reached ∼92.3% when the vertical drift exceeded 30 m/s in the presence of LSWS. These results suggested that the presence of LSWS constitutes a precondition for ESF generation during this studying interval, whereas a strong PSSR acts as a favorable condition.
Source: Geophysical Research Letters
DOI: 10.1029/2025gl120013
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $3,190
Funder: Chinese Academy of Sciences
Award: G7275436811
OpenAlex ID: W7166741042
