Morphological and Spectral Features of Ionospheric Structures at E- and F-Region Altitudes over Poker Flat Analyzed Using Modeling and Observations

Abstract

Electron density irregularities in the ionosphere modify the phase and amplitude of trans-ionospheric radio signals. We aim to characterize the spectral and morphological features of E- and F-region ionospheric irregularities likely to produce these fluctuations or “scintillations”. To characterize them, we use a three-dimensional radio wave propagation model—“Satellite-beacon Ionospheric scintillation Global Model of upper Atmosphere” (SIGMA), along with the scintillation measurements observed by a cluster of six Global Positioning System (GPS) receivers called Scintillation Auroral GPS Array (SAGA) at Poker Flat, AK. An inverse method is used to derive the parameters that describe the irregularities by estimating the best fit of model outputs to GPS observations. We analyze in detail one E-region and two F-region events during geomagnetically active times and determine the E- and F-region irregularity characteristics using two different spectral models as input to SIGMA. Our results from the spectral analysis show that the E-region irregularities are more elongated along the magnetic field lines with rod-shaped structures, while the F-region irregularities have wing-like structures with irregularities extending both along and across the magnetic field lines. We also found that the spectral index of the E-region event is less than the spectral index of the F-region events. Additionally, the spectral slope on the ground at higher frequencies is less than the spectral slope at irregularity height. This study describes distinctive morphological and spectral features of irregularities at E- and F-regions for a handful of cases performed using a full 3D propagation model coupled with GPS observations and inversion.

Model‐Based Investigation of Electron Precipitation‐Driven Density Structures and Their Effects on Auroral Scintillation

“…We used the same technique in Vaggu et al. (2023) to study the morphology of auroral scintillation producing irregularities over Poker Flat. The physics‐based model GEMINI was coupled with SIGMA to study scintillation in polar cap patches with gradient‐drift instability as the underlying instability mechanism (K. B. Deshpande & Zettergren, 2019; Spicher et al., 2020).…”

“…K. Deshpande et al (2016) studied auroral and polar cap scintillation, where spectral models were used to create ionospheric structuring and an inverse method with SIGMA was employed to understand the physics of irregularities. We used the same technique in Vaggu et al (2023) to study the morphology of auroral scintillation producing irregularities over Poker Flat. The physics-based model GEMINI was coupled with SIGMA to study scintillation in polar cap patches with gradient-drift instability as the underlying instability mechanism (K. B.…”