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@InProceedings{RodríguezGómesVieiDalLPala:2018:CoElDe,
               author = "Rodr{\'{\i}}guez G{\'o}mes, Jenny Marcela and Vieira, 
                         Lu{\'{\i}}s Eduardo Antunes and Dal Lago, Alisson and Palacios, 
                         J.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Universidad de Alcal{\'a}}",
                title = "Coronal electron density temperature and solar spectral irradiance 
                         during solar cycles 23 and 24",
                 year = "2018",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 7. (SBGEA)",
             abstract = "Plasma parameters such as the electron density and temperature 
                         play a key role in the dynamics of the solar atmosphere. These 
                         characteristics are important in solar physics because they can 
                         help us to understand the physics of the solar corona, the 
                         ultimate goal being the reconstruction of the electron density and 
                         temperature distributions in the solar corona. We present a 
                         physics-based model to reconstruct the density, temperature, and 
                         emission in the EUV band. This model, called COronal DEnsity and 
                         Temperature (CODET), is composed of a flux transport model, an 
                         extrapolation model, an emission model, and an optimization 
                         algorithm. The CODET model parameters were constrained by 
                         comparing the models output to the TIMED/SEE record instead of 
                         direct observations because it covers a longer time interval than 
                         the direct solar observations currently available. The most 
                         important results of the current work are the recovery of SSI 
                         variability in specific wavelengths in the EUV band, as well as 
                         the variations in density and temperature during the solar cycle 
                         23 and 24, through the solar atmosphere with the CODET model.",
  conference-location = "Santa Maria, RS",
      conference-year = "05-09 nov",
             language = "pt",
           targetfile = "rodriguez_coronal.pdf",
        urlaccessdate = "23 jan. 2021"
}


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