Ionosonde-f0F2 measurements and corresponding GNSS TEC measurements have been analysed. Available f0F2 and TEC data respectively obtained from a pair of ionosonde and GNSS receiver stations of a mid-latitude station, named MO155, located in Moscow (55.8˚N, 37.2˚E), for 2010 and 2014 was used. Data for two years were respectively used in the study to represent years of low and high solar activity. A significant relation between the ionosonde-f0F2 measurements and the corresponding GNSS-VTEC measurements with correlation coefficients above 0.8 was observed for both periods. The f0F2/TEC ratios, for the MO155 station illustrated, are typically in the range of about 0.2 to 1.6 Mhz/TECU during the low solar activity period and 0.2 to 2.5 Mhz/TECU during the high solar activity period. The ratio is lower during the day-time, and higher during the nights and early mornings. The analysis of the four seasons for both periods (low solar activity and high solar activity) reveals a strong relationship between TEC and f0F2 in all the seasons. Significantly, summer season appear to have a different trend from all other seasons with a relatively low correlation. The relationship between TEC and f0F2 seem to be stronger during period of high solar activity than period of low solar activity. Results from the work indicate that the relationship between f0F2 and TEC is mostly dependent on the seasons, followed by the level of solar activity, and then the local time. It was shown that the relationship between f0F2 and TEC is not purely monotonic as suggested earlier; but that this relationship depends on factors like the season, level of solar activity, and local time. Considering the strong relationship between f0F2 and TEC, the study affirms the method of using TEC as a proxy for f0F2 estimation.
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