@InProceedings{SilvaDMRMPBS:2021:IoTERe,
               author = "Silva, R{\'e}gia Pereira da and Denardini, Clezio Marcos and 
                         Marques, M. S. and Resende, Laysa Cristina Ara{\'u}jo and Moro, 
                         Juliano and Pican{\c{c}}o, Giorgio Arlan da Silva and Borba, G. 
                         L. and Santos, Marcos Aur{\'e}lio Ferreira dos",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Universidade Federal 
                         do Rio Grande do Norte (UFRN)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Universidade Federal do Rio Grande do Norte (UFRN)} 
                         and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Ionospheric TEC responses to HILDCAAs intervals",
                 year = "2021",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 8. (SBGEA)",
             abstract = "The High-Intensity Long-Duration and Continuous AE Activities 
                         (HILDCAA) intervals are capable of causing a global disturbance in 
                         the terrestrial ionosphere. However, the ionospheric storms 
                         behavior due to these intervals is still not widely understood. In 
                         the current study, we seek to comprise the HILDCAAs disturbance 
                         time effects in the Total Electron Content (TEC) values with 
                         respect to the quiet days pattern analyzing local time and 
                         seasonal dependences, and the influences of the solar wind 
                         velocity to a sample of ten intervals occurred in 2015 and 2016 
                         years. The main results showed that the hourly distribution of the 
                         disturbance TEC may vary substantially between one HILDCAA 
                         interval and another. It was found an equinoctial anomaly since 
                         the equinoxes represent more ionospheric TEC responses than the 
                         solstices. Regarding the solar wind velocities, although HILDCAA 
                         intervals are associated with High-Speed Streams, this association 
                         does not present a direct relation to TEC disturbances magnitudes 
                         in low and equatorial latitudes.",
  conference-location = "Online",
      conference-year = "22-26 mar.",
             language = "en",
        urlaccessdate = "09 maio 2024"
}