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GPS L1-Frequency Observations of Equatorial Scintillations and Irregularity Zonal Velocities

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Abstract

In this work, the climatology of ionospheric scintillations at global positioning system (GPS) L-band frequency and the zonal drift velocities of scintillation-producing irregularities were depicted for the equatorial observatory of São Luis (2.33°S; 44.21°W; dip latitude 1.3°S), Brazil. This is the first time that the hourly, monthly, and seasonal variations of scintillations and irregularity zonal drifts at São Luis were characterized during periods of different solar activity levels (from December 1998 to February 2007). The percentage occurrence of scintillations at different sectors of the sky was also investigated, and the results revealed that the scintillations are more probable to be observed in the west sector of the sky above São Luis, whereas the north–south asymmetries are possibly related to asymmetries in the plasma density distribution at off-equatorial latitudes. The scintillations on GPS signals occurred more frequently around solar maximum years, but it is also clear from the results of a strong variability in the scintillation activity in the years with moderate solar flux during the descending phase of the solar cycle. The equatorial scintillations occur predominantly during pre-midnight hours with a broad maximum near the December solstice months. In general, weak level of scintillations (S 4 index between 0.2 and 0.4) dominated at all seasons; however, during the winter months around solar maximum years (although the scintillation occurrence is extremely low), stronger levels of scintillations (S 4 > 0.6) may occur at comparable rate with the weak scintillations. The irregularity zonal velocities, as estimated from the GPS spaced-receiver technique, presented a different scenario for the two seasons analyzed; during the equinoxes, the magnitude of the zonal velocities appeared not to change with the solar activity, whereas during the December solstice months, the larger magnitudes were observed around solar maximum years. Other relevant aspects of the observations are highlighted and discussed.

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Acknowledgments

This work was partially supported by Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) under Processes No. 2012/06598-2 and 2008/04892-5, by Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) under Process No. AEX9761/11-0, and Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) under Grant No. 308017/2011-0.

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  1. Laboratório de Física e Astronomia, IP&D, Universidade do Vale do Paraíba, São José dos Campos, São Paulo, 12244-000, Brazil

    Marcio T. A. H. Muella

  2. Aeronomy Division, National Institute for Space Research, São José dos Campos, São Paulo, 12227-010, Brazil

    Eurico R. de Paula & Olusegun F. Jonah

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  1. Marcio T. A. H. Muella
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  2. Eurico R. de Paula
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  3. Olusegun F. Jonah
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Correspondence to Marcio T. A. H. Muella.

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Muella, M.T.A.H., de Paula, E.R. & Jonah, O.F. GPS L1-Frequency Observations of Equatorial Scintillations and Irregularity Zonal Velocities. Surv Geophys 35, 335–357 (2014). https://doi.org/10.1007/s10712-013-9252-0

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