@InProceedings{SousasantosAMKSSSS:2018:RoSeSo,
               author = "Sousasantos, Jonas and Abdu, Mangalathayil Ali and Moraes, A. O. 
                         and Kherani, Esfhan Alam and Sobral, Jos{\'e} Humberto Andrade 
                         and Silva, A. L. A. and Silva, R. P. da and Salles, L. A.",
          affiliation = "{Instituto Tecnol{\'o}gico de Aeron{\'a}utica (ITA)} and 
                         {Instituto Tecnol{\'o}gico de Aeron{\'a}utica (ITA)} and 
                         {Instituto de Aeron{\'a}utica e Espa{\c{c}}o (IAE)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Tecnologico 
                         de Aeron{\'a}utica (ITA)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Tecnologico de Aeron{\'a}utica 
                         (ITA)}",
                title = "Different seeds, different outcomes: the role of the seeding 
                         source in the plasma bubble morphology",
                 year = "2018",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 7. (SBGEA)",
             abstract = "Across the years, several numerical simulations studies on the 
                         Equatorial Plasma Bubble (EPB) phenomenon have been carried out. 
                         Among the most prominent discussions in this field of space 
                         research is the seeding source question. Scientists have argued in 
                         favor of several different mechanisms capable to trigger the 
                         so-called collisional interchange instability leading to the 
                         formation of the EPB structures in the nonlinear regime. Density 
                         perturbations, gravity waves, prereversal vertical drift gradient, 
                         etc., are examples of elements which belong to the set of 
                         candidates for seeding source mechanism proposed through the 
                         decades. In this work, some of these seeding sources are tested 
                         using a mathematical and computer modeling to solve the set of the 
                         hydromagnetic equations of the state. The results suggest a strong 
                         influence of the seed in the outcome, i.e., different mechanisms 
                         cause dissimilar mature EPB structures rather than akin 
                         structures. The implication of this result is that not only the 
                         ionospheric ambient influences the evolution of the EPB structures 
                         but also that the nature of seeding source action during the 
                         unborn stage of the EPB structure may bring substantial 
                         consequences in the EPB morphology.",
  conference-location = "Santa Maria, RS",
      conference-year = "05-09 nov",
             language = "pt",
        urlaccessdate = "04 jun. 2024"
}