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A statistical study on the <i>F</i><sub>2</sub> layer vertical variation during nighttime medium‐scale traveling ionospheric disturbances
17
Citations
49
References
2017
Year
GeophysicsUpper AtmosphereGeospace PhysicsVertical VariationPerturbation ComponentEngineeringAtmospheric ScienceLayer Peak HeightIonosphereMagnetospheric PhysicsStatistical StudySpace Plasma PhysicSolar-terrestrial InteractionIonospheric DisturbancesTotal Electron ContentSpace WeatherEarth ScienceLower Atmosphere
Abstract A statistical study on the relationship between the perturbation component (ΔTEC (total electron content)) and the F 2 layer peak height ( h m F 2 ) during nighttime medium‐scale traveling ionospheric disturbances is presented. The results are obtained by using a time‐dependent computerized ionospheric tomography (CIT) technique. This was realized by using slant total electron content observations from a dense Global Positioning System receiver network over Japan (with more than 1000 receivers), together with a multiplicative algebraic reconstruction technique. Reconstructions from CIT were validated by using ionosonde and occultation measurements. A total of 36 different time snapshots of the ionosphere when medium‐scale traveling ionospheric disturbances (MSTIDs) were eminent were analyzed. These were obtained from a data set covering years from 2011 to 2014. The reconstructed surface wavefronts of ΔTEC and h m F 2 structure were found to be aligned along the northwest‐southeast direction. These results confirm that nighttime MSTIDs are driven by electrodynamic forces related to Perkins instability which explains the northwest‐southeast wavefront alignment based on the F region electrodynamics. Furthermore, from the statistical analysis h m F 2 varied quasiperiodically in altitude with dominant peak‐to‐peak amplitudes between 10 and 40 km. In addition, ΔTEC and h m F 2 were 60% anticorrelated.
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