@InProceedings{SantosSantNascViei:2021:EUEmX8,
               author = "Santos, T. L. A. and Santos, J. C. and Nascimento, B. M. and 
                         Vieira, Luis Eduardo Antunes",
          affiliation = "{Universidade Tecnol{\'o}gica Federal do Paran{\'a} (UTFPR)} and 
                         {Universidade Tecnol{\'o}gica Federal do Paran{\'a} (UTFPR)} and 
                         {Universidade Tecnol{\'o}gica Federal do Paran{\'a} (UTFPR)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "EUV emissions of a X8.2 Flare",
                 year = "2021",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 8. (SBGEA)",
             abstract = "Solar flares are defined observationally as an increase of 
                         electromagnetic emission in different wavelengths. On September 
                         10th 2017 an intense (X8.2 class) flare occurred at the Suns limb, 
                         associated to active region NOAA 12673. The GOES x-ray flux 
                         sensors pointed that the peak of the flare was at 16:54 UT. In 
                         this work we used AIA measurements, on board the SDO satellite, to 
                         investigate the temporal and spatial variations of seven EUV bands 
                         (94, 131, 171, 193, 211, 304 e 335). Our research consist in using 
                         the AIA images to build temporal series of total emission and 
                         vertical profiles for a period of 6 hours around the peak of the 
                         flare, in order to understand how the energy is released and 
                         transported in the solar atmosphere. The results obtained are 
                         compared with the CSHKP standard flare model. This work will help 
                         us to understand how the energy release and the plasma heating 
                         processes affect the energy distribution in the solar atmosphere 
                         and if the processes is in accordance with the standard model.",
  conference-location = "Online",
      conference-year = "22-26 mar.",
             language = "en",
        urlaccessdate = "09 maio 2024"
}