Comparison of low latitude F region peak densities, heights and equatorial E×B drift from IRI with observational data and the Sheffield University plasmasphere ionosphere model

• Published in: Advances in space research 2003, Vol.31 (3), p.501-505
• Main Authors: Souza, J.R., Bailey, G.J., Abdu, M.A., Batista, I.S.
• Format: Article
• Language: English
• ISSN: 0273-1177; 1879-1948
• DOI: 10.1016/S0273-1177(03)00050-4

Observed values of the critical frequency and real height of the ionospheric F-region peak (foF2 and hmF2, respectively) over Fortaleza (4° S, 38° W) and Cachoeira Paulista (22.5° S, 45° W) near solar minimum are compared with their values calculated by the International Reference Ionospheric Model (IRI). A comparison between the equatorial E× B drift velocities represented by IRI and those obtained by a method that uses the Sheffield University Plasmasphere Ionosphere Model (SUPIM) has also been carried out. In general, the values of foF2 and hmF2 calculated by IRI using the International Radio Consultive Committee (CCIR) maps show better agreement with the observed values than do those obtained using the International Union of Radio Science (URSI) maps for both stations, Fortaleza and Cachoeira Paulista. Equatorial E× B drift velocities calculated by IRI/Scherliess and Fejer (1999) have presented values different from those calculated by SUPIM mainly during evening and nighttime for December solstice and equinox conditions.