@InProceedings{KheraniPaMuCaReSm:2008:ObGPNe,
               author = "Kherani, E. A. and Paula, Eurico Rodrigues de and Muella, Marcio 
                         Tadeu de Assis Honorato and Campos, Alessandro Augusto Nunes and 
                         Rezende, Luiz Felipe de Campos and Smorigo, Paulo Flabiano",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "The large TEC fluctuations near the Equatorial ionization anomaly 
                         during the equatorial spread F: observation from the GPS network 
                         over Brazil and simulation",
            booktitle = "Proceedings...",
                 year = "2008",
         organization = "International Symposium on Equatorial Aeronomy, 12.",
             abstract = "To monitor the scintillation induced by ionospheric 
                         irregularities, a number of GPS receivers are deployed over 
                         Brazil. They provide the real-time distribution of scintillation 
                         activity and TEC fluctuations induced by the equatorial spread F. 
                         We has found that the TEC fluctuations is large near the 
                         equatorial ionization anomaly (EIA) as compared to the equatorial 
                         region where they are originally generated. The large TEC 
                         fluctuations near EIA region needs an explanation. To do so, we 
                         carry out the 3D numerical simulation of spread F bubble including 
                         the dynamics parallel and perpendicular to the magnetic field. The 
                         simulation shows that the large ionospheric density gradient in 
                         the equatorward boundary of EIA region is probably responsible for 
                         the observed large TEC fluctuations.",
  conference-location = "Crete, Greece",
      conference-year = "18-24 may",
                label = "self-archiving-INPE-MCTIC-GOV-BR",
             language = "en",
           targetfile = "kherani_large.pdf",
        urlaccessdate = "28 abr. 2024"
}