Quiet Time Variation of Ionosphere Parameters near Equator | Chapter 2 | Advances and Trends in Physical Science Research Vol. 2

In recent, ionosphere has been intensively investigated by analyzing data variability and or improving existing models for now casting and or forecasting reasons. Therefore, the investigation of f2 layer critical frequency (fof2) parameter by means of the 2012 version of iri (international reference ionosphere) model and tiegcm (thermosphere ionosphere electrodynamics general circulation model) is required. The present study appreciates the estimation of TIEGCM (Thermosphere Ionosphere Electrodynamics General Circulation Model) and that of the 2012 version of IRI in African Equatorial Ionisation Anomaly (EIA) region through the diurnal variation of F2 layer critical frequency (foF2). The comparison made between data and theoretical values carried out from TIEGCM and IRI-2012 during solar cycle minimum and maximum phases and under quiet time condition over seasons. Data concern solar cycle 22 foF2 data of Ouagadougou station (Lat: 12.4° N; Long: 358.5°E, dip: 1.43°N for 2013) provided by Télécom Bretagne. Quiet time condition is determined by Aa inferior or equal to 20 nT and solar cycle maximum, and minimum phases correspond to sunspot number Rz superior to 100 and Rz inferior to 20, respectively. Seasons are estimated by considering December as winter month, March as spring month, June as summer month and September as autumn month. Models predictions are better during solar maximum than during solar minimum and strongly dependent on pre-sunrise and post-sunset periods. The seasonal Hourly quiet time foF2 is given by the arithmetic mean values of the five quietest day hourly values. Data profiles show noon bite out a profile with more and less pronounced morning or afternoon peak in equinox and that during solar maximum and that also in solar minimum except during solstice where the profile fairly is dome or plateau. During solar minimum, both models present a more or less pronounced afternoon peak with more or less deep trough between 1000 LT and 1400 LT. During solar maximum, in general, TIEGCM shows afternoon peak and IRI-2012 present plateau profile. This result exhibits the non-well estimation of the dynamic process of this region. Model accuracy is highlighted by the Mean Relative Error (MRE) values. These values show a better prediction for IRI-2012 except in September for both solar cycle phases involved. The non-good prediction of TIEGCM is observed in December during solar minimum and in June during solar maximum. This study shows that running IRI model enables to show that foF2 time variations present “reversed profiles” on minimum and “plateau profile” on maximum solar cycle phases. It also shows winter anomaly on foF2 profiles.  These different conclusions have been previously found by other authors. This work also reports winter anomaly on foF2 parameter. The closed link between foF2 and TEC time variations is carried out. (Winter anomaly on TEC). The study shows Total electron contents effects on critical frequency of radio waves in the ionosphere layer.

Biography of author(s)

Emmanuel Nanema
Research Laboratory for Energy and Space Weather, University of Koudougou, Koudougou BP 376, Burkina Faso and Research Institute of Applied Sciences and Technologies (IRSAT) CNRST, 03 BP 7047 Ouagadougou 03, Burkina Faso

Frédéric Ouattara
Research Laboratory for Energy and Space Weather, University of Koudougou, Koudougou BP 376, Burkina Faso.

Read full article: http://bp.bookpi.org/index.php/bpi/catalog/view/25/60/148-1
View Volume: https://doi.org/10.9734/bpi/atpsr/v2

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