@InProceedings{FigueiredoMWTSERS:2023:SeInGe,
               author = "Figueiredo, Cosme Alexandre Oliveira Barros and Miranda, Rodrigo 
                         A. and Wrasse, Cristiano Max and Takahashi, Hisao and Silva, Diego 
                         Barros and Egito, F{\'a}bio and Rosa, Ge{\^a}ngelo de Matos and 
                         Sampaio, Antonio H{\'e}lder Rodrigues",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Secondary instability generated on the equatorial plasma bubbles 
                         wall due to an interaction with the midnight brightness wave",
            booktitle = "Anais...",
                 year = "2023",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 9.",
             abstract = "Interaction between Equatorial Plasma Bubbles (EPBs) and midnight 
                         Brightness wave (MBW) was observed over Bom Jesus da Lapa (13.3° 
                         S, 43.5° W; Quasi-Dipole geomagnetic latitude of 14.1° S), using 
                         OI 630 nm all-sky images. On the night of December 22nd, 2019, an 
                         EPB was seen propagating eastward in its fossil stage until it 
                         interacted with an MBW. After the interaction, the west walls of 
                         EPBs generated secondary instabilities that can be associated with 
                         gradient drift instability (GDI) and/or KelvinHelmholtz 
                         instabilities (KHI). We suggest that the MBW contributed to 
                         generate a shear in the EPBs walls due to changes in the 
                         thermospheric dynamics, such as neutral wind in the F layer 
                         height. Furthermore, spectral analysis of the all-sky images 
                         suggests that GDI and/or KHI generated turbulence and helped to 
                         dissipate the EPBs.",
  conference-location = "Araguatins, TO",
      conference-year = "19-23 jun. 2023",
             language = "en",
           targetfile = "s40623-023-01892-7.pdf",
        urlaccessdate = "04 jun. 2024"
}