Abstract M(3000)F2 estimation of hmF2 based on four different formulated models viz: (1) (2) , (3) and (4) at an equatorial station in West Africa during low solar activity period (1995) are used to validate its conformity with observed and International Reference Ionosphere (IRI) model. Local time analyses of data from fifteen (15) selected days during the January and July solstices and April and October equinoxes are used. The results obtained show that the M(3000)F2 estimation of hmF2 from the ionosonde-measured values using the Ionospheric Prediction Service (IPS-42) sounder compared to the observed values which were deduced using an algorithm from scaled virtual heights of quiet day ionograms are highly correlated with Bilitza model. International Reference Ionosphere (IRI 2007) model for the equatorial region also agrees with the formulation developed by for the four different seasons of the year. hmF2 is highest (425km) in summer (June solstice) season and lowest (386km) in autumn (September equinox) season with daytimes peaks occurring at 1100–1200 LT during the solstices and at 1000 LT during the equinoxes respectively. Also, the post-sunset peaks are highest (362km) at the spring (March equinox) and lowest (308km) at the summer (June solstice) both occurring between 1800 and 2000 LT.
Equatorial M(3000)F2 estimation of F2-layer models peak heights during low solar activity
Advances in Space Research ; 49 , 4 ; 711-715
2011-11-24
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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