@InProceedings{CândidoBKSCOBA:2022:OvBrLo,
               author = "C{\^a}ndido, Cl{\'a}udia and Becker Guedes, F{\'a}bio and 
                         Klausner, Virginia and Santos, Stella Moraes and Chingarandi, 
                         Frank Simbarashe and Olusayo, Osanyin Taiwo and Orue and Yenca and 
                         Migoya and Borries, Claudia and Abaidoo, Samuel",
          affiliation = "{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} 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)} and 
                         {Abdus Salam International Center for Theoretical Physics} and 
                         {German Aerospace Center (DLR)} and {Universidade do Vale do 
                         Para{\'{\i}}ba (UNIVAP)}",
                title = "An overview of the brazilian low latitude ionospheric response to 
                         space weather events during the declining phase of solar cycle 
                         24",
                 year = "2022",
         organization = "COSPAR Scientific Assembly, 44.",
             abstract = "This study shows an overview of the Brazilian low-latitude 
                         ionospheric response during the declining phase and solar minimum 
                         of solar cycle 24. It is well-known that during the descending 
                         phase, solar low-latitude coronal holes are responsible by solar 
                         wind high-speed streams, HSSs, and corotating interaction regions 
                         CIRs-driven geomagnetic storms. Although distinct in nature, 
                         intensity, and duration of their counterpart Coronal Mass 
                         Ejection, CMEs/ICMEsstorms, these solar events can significantly 
                         change the low-latitude ionosphere for several days. By using 
                         multiple ground-based and satellite instrumental techniques, we 
                         analyzed the variation of the Total Electron Content, TEC, its 
                         deviation from the quietest average days behavior, and other 
                         ionospheric parameters and indices. VTEC intensifications can be 
                         as high as 400.",
  conference-location = "Athens, Greece",
      conference-year = "16-24 July 2022",
             language = "en",
           targetfile = "C1.5-0003-22-oral.pdf",
        urlaccessdate = "03 maio 2024"
}