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VTEC behavior in the American sector during high solar activity

The behavior of the vertical total electron content (VTEC) obtained from GPS signals received during the high solar activity year 1999 at stations placed in the American sector, is reported. The considered latitude range extends from 18.4 to -64.7 and the longitude ranges from 281.3 to 297.7. Median...

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Detalles Bibliográficos
Autores principales: Ezquer, R G, Azpilicueta, F, Brunini, C, Conicet, Meza, A, Mosert, M, Radicella, S M
Lenguaje:eng
Publicado: Trieste Univ. Abdus Salam Int. Centre Theor. Phys. 2002
Materias:
Acceso en línea:http://cds.cern.ch/record/746989
Descripción
Sumario:The behavior of the vertical total electron content (VTEC) obtained from GPS signals received during the high solar activity year 1999 at stations placed in the American sector, is reported. The considered latitude range extends from 18.4 to -64.7 and the longitude ranges from 281.3 to 297.7. Median, lower and upper quartiles are used to specify variability, because they have the advantage of being less affected by large deviations that can occur during magnetic storms. The results show that the VTEC values corresponding to equinox are greater than those of solstice and that, the highest VTEC values are observed at low latitude stations. In general, the variability during daylight hours is about 30% of median or less, and that observed for nighttime hours is greater than the mentioned percentage, particularly at last hours of the night near the northern peak of the equatorial anomaly.