@InProceedings{FigueiredoWTOSBPS:2021:EvInEq,
               author = "Figueiredo, Cosme Alexandre Oliveira Barros and Wrasse, Cristiano 
                         Max and Takahashi, Hisao and Otsuka, Y. and Shiokawa, K. and 
                         Buriti, R. and Paulino, I. and Silva, D.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Nagoya University} and {Nagoya 
                         University} and {Universidade Federal de Campina Grande (UFCG)} 
                         and {Universidade Federal de Campina Grande (UFCG)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "Evidence of interaction between Equatorial Plasma Bubble, 
                         Medium-scale Traveling Ionospheric Disturbances, and Midnight 
                         Brightness Wave",
                 year = "2021",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 8. (SBGEA)",
             abstract = "Observation of equatorial plasma bubbles (EPBs), mediumscale 
                         traveling ionospheric disturbance (MSTID), and midnight brightness 
                         wave (MBW) were made using the OI 630 nm emission by an All-Sky 
                         imager located at Cachoeira Paulista, Brazil (22.7\◦S, 
                         45.0\◦W, magnetic dip latitude \∼20\◦S, 
                         referring to 2015) on the night of September 17-18, 2015. The EPBs 
                         were observed moving eastward while the MSTID propagated 
                         northwestward with the wavefront aligned to southwest-northeast. 
                         On the other side, the MBW was observed moving to south-southwest. 
                         After the interaction between the MSTIDS and the EPBs, the latter 
                         became tilted, grew and narrowed. This effect could be associated 
                         to the ExB drift and also to changes in the neutral wind. 
                         Furthermore, an MBW also interacts with EPB and fills the EPB edge 
                         with plasma transforming it into a bright structure.",
  conference-location = "Online",
      conference-year = "22-26 mar.",
             language = "en",
        urlaccessdate = "04 maio 2024"
}