@Article{CarmoDDFWRSMCPSWLL:2023:EqPlBu,
               author = "Carmo, Carolina de Sousa do and Dai, L. and Denardini, Clezio 
                         Marcos and Figueiredo, Cosme Alexandre Oliveira Barros and Wrasse, 
                         Cristiano Max and Resende, Laysa Cristina Ara{\'u}jo and Silva, 
                         Diego Barros and Moro, Juliano and Chen, Sony Su and 
                         Pican{\c{c}}o, Giorgio Arlan da Silva and Silva, R{\'e}gia 
                         Pereira da and Wang, C. and Li, H. and Liu, Z.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Chinese 
                         Academy of Sciences} 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 {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 
                         {Chinese Academy of Sciences} and {Chinese Academy of Sciences} 
                         and {Chinese Academy of Sciences}",
                title = "Equatorial plasma bubbles features over the Brazilian sector 
                         according to the solar cycle and geomagnetic activity level",
              journal = "Frontiers in Astronomy and Space Sciences",
                 year = "2023",
               volume = "10",
                pages = "e1252511",
             keywords = "ionosphere, equatorial plasma bubbles, space weather, solar cycle, 
                         magnetic activity.",
             abstract = "Equatorial plasma bubbles (EPBs) can lead to signal degradation, 
                         affecting the measurement accuracy. Studying EPBs and their 
                         characteristics has gained increasing importance. The 
                         characteristics of EPBs were investigated using the rate of total 
                         electron content (TEC) index (ROTI) maps under different solar and 
                         magnetic activity conditions during two periods: July 2014-July 
                         2015 (solar maximum activity with F10.7: 145.9 x 10(-22)W center 
                         dot m(-2)center dot Hz(-1)) and July 2019-July 2020 (solar minimum 
                         activity with F10.7: 69.7 x 10(-22)W center dot m(-2)center dot 
                         Hz(-1)). We also divided this analysis according to the magnetic 
                         activity levels based on Kp and Dst (disturbance storm time) 
                         indices, classified as follows: quiet+ (Kp <= 3 and Dst >-30 nT), 
                         quiet- (Kp <= 3 and Dst <-30 nT), disturbed weak (-50 nT.",
                  doi = "10.3389/fspas.2023.1252511",
                  url = "http://dx.doi.org/10.3389/fspas.2023.1252511",
                 issn = "2296-987X",
                label = "self-archiving-INPE-MCTIC-GOV-BR",
             language = "en",
           targetfile = "fspas-10-1252511.pdf",
        urlaccessdate = "08 maio 2024"
}