@Article{PicançoDNRCCBR:2022:StEqLo,
               author = "Pican{\c{c}}o, Giorgio Arlan da Silva and Denardini, Clezio 
                         Marcos and Nogueira, Paulo Alexandre Bronzato and Resende, Laysa 
                         Cristina Ara{\'u}jo and Carmo, Carolina de Sousa and Chen, Sony 
                         Su and Barbosa Neto, Paulo Fran{\c{c}}a and Romero Hernandez, 
                         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 {Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {Universidad Aut{\'o}noma de Nuevo Le{\'o}n}",
                title = "Study of the equatorial and low-latitude total electron content 
                         response to plasma bubbles during solar cycle 24-25 over the 
                         Brazilian region using a Disturbance Ionosphere indeX",
              journal = "Annales Geophysicae",
                 year = "2022",
               volume = "40",
               number = "4",
                pages = "503--517",
                month = "July",
             abstract = "This work uses the Disturbance Ionosphere indeX (DIX) to evaluate 
                         the ionospheric responses to equatorial plasma bubble (EPB) events 
                         from 2013 to 2020 over the Brazilian equatorial and low latitudes. 
                         We have compared the DIX variations during EPBs to ionosonde and 
                         All-Sky Imager data, aiming to evaluate the physical 
                         characteristics of these events. Our results show that the DIX was 
                         able to detect EPB-related TEC disturbances in terms of their 
                         intensity and occurrence times. Thus, the EPB-related DIX 
                         responses agreed with the ionosphere behavior before, during, and 
                         after the studied cases. Finally, we found that the magnitude of 
                         those disturbances followed most of the trends of solar activity, 
                         meaning that the EPB-related total electron content variations 
                         tend to be higher (lower) in high (low) solar activity.",
                  doi = "10.5194/angeo-40-503-2022",
                  url = "http://dx.doi.org/10.5194/angeo-40-503-2022",
                 issn = "0992-7689",
             language = "en",
           targetfile = "angeo-40-503-2022.pdf",
        urlaccessdate = "20 maio 2024"
}