@InProceedings{PicançoDNRCMNMCBR:2022:DyEqPl,
               author = "Pican{\c{c}}o, Giorgio Arlan da Silva and Denardini, Clezio 
                         Marcos and Nogueira, Paulo and Resende, Laysa Cristina Ara{\'u}jo 
                         and Carmo, Carolina de Sousa and Meza, Amalia and Natali, Maria 
                         Paula and Mendoza, Luciano and Chen, Sony Su and Barbosa Neto, 
                         Paulo Fran{\c{c}}a and Romero Hern{\'a}ndez, Esmeralda",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Federal de 
                         S{\~a}o Paulo (IFSP)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Universidad Nacional de La Plata} and {Universidad 
                         Nacional de La Plata} and {Universidad Nacional de La Plata} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and UNAM",
                title = "Dynamics of equatorial plasma bubbles over the brazilian sector 
                         observed using disturbance ionosphere index (DIX) maps",
                 year = "2022",
         organization = "COSPAR Scientific Assembly, 44.",
             abstract = "In this work, we use Disturbance Ionosphere indeX (DIX) maps to 
                         evaluate the dynamic characteristics of Equatorial Plasma Bubbles 
                         (EPBs) over the Brazilian sector. In this context, we analyze the 
                         latitudinal and longitudinal temporal evolution of EPBs by 
                         selecting cases within a time series of DIX maps and comparing 
                         them to All-Sky Imager (ASI) OI 630 nm airglow data. From that 
                         analysis, we estimate some physical characteristics of those 
                         events, such as latitudinal extension. Our results show that the 
                         bubbles observed as disturbances on the DIX maps are in agreement 
                         with the EPB signatures observed on the ASI images. Finally, we 
                         also found that the magnitude of those disturbances followed most 
                         of the trend of solar activity, meaning that the EPB-related 
                         plasma variations tend to be higher (lower) in high (low) solar 
                         activity.",
  conference-location = "Athens, Greece",
      conference-year = "16-24 July 2022",
             language = "en",
           targetfile = "C1.1-0005-22-oral.pdf",
        urlaccessdate = "20 maio 2024"
}