Publication | Open Access
Climatology of medium-scale traveling ionospheric disturbances observed by a GPS network in central China
129
Citations
43
References
2011
Year
EngineeringSolar ConvectionGlobal Navigation Satellite SystemSolar-terrestrial InteractionGps NetworkData AssimilationEarth ScienceGeophysicsGeospace PhysicsAtmospheric ScienceCentral ChinaSolar ActivityMeteorologyGeographyIonospheric DisturbancesSpace WeatherSunspot StudiesClimatologySolar Minimum PeriodDaytime MstidsSolar VariabilitySatellite MeteorologyPhase VelocityIonosphere
[1] The 15-month climatology of medium-scale traveling ionospheric disturbances (MSTIDs) during a solar minimum period has been constructed from observations of a dense GPS receiver array in Central China. In total, 793 MSTID events are identified, with peaks in occurrence at 1500 LT and 0100 LT. The occurrence of MSTIDs decreases following an increase in geomagnetic activity, with 46% of the MSTIDS occurring in the daytime. Daytime MSTIDs are characterized by a major occurrence maximum around the winter solstice and by an equatorward propagation direction. The period, phase velocity, azimuth, and amplitude of daytime MSTIDs are 20–60 min, 100–400 m/s, 130°–270°, and 0.8–1.5%, respectively. The remaining 54% of the MSTIDs occurred at night, and were characterized by a peak in occurrence at the summer solstice and by a southwestward propagation direction. The period, phase velocity, azimuth, and amplitude of nighttime MSTIDs are 20–70 min, 50–230 m/s, 170°–300°, and 2–7%, respectively. The propagation directions and the seasonal behaviors support the view that daytime MSTIDs are an ionospheric manifestation of atmospheric gravity waves from the lower atmosphere, while a possible excitation mechanism of nighttime MSTIDs is the electrodynamics process caused by plasma instability in the F layer.
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