@InProceedings{BravoSouMarVenBar:2024:EvIoIm,
               author = "Bravo, Manuel and Souza, Jonas Rodrigues de and 
                         Mart{\'{\i}}nez-Ledesma, Miguel and Venchiarutti, 
                         Valent{\'{\i}}n and Barb{\'a}s, Blas de Haro",
          affiliation = "{Universidad Adventista de Chile} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Universidad Adventista de Chile} 
                         and {Universidad Adventista de Chile} and {Universidad Adventista 
                         de Chile}",
                title = "Evaluation of Ionospheric Impact Prediction during the Solar 
                         Eclipse of October 14, 2023",
            booktitle = "Proceedings...",
                 year = "2024",
         organization = "Conferencia Latinoamericana de Geof{\'{\i}}sica Espacial, 14.",
             abstract = "Solar eclipses are an excellent opportunity for ionospheric 
                         researchers to use as a natural ionospheric laboratory. The 
                         production of ions-electrons in the ionosphere is due to the 
                         photoionization process that depends directly on solar radiation. 
                         During a solar eclipse, the gradual decrease in solar radiation to 
                         totality (in some cases) creates a geographic window (minutes to 
                         hours) of nighttime conditions during daylight hours. Under these 
                         conditions it is possible to evaluate and study the response of 
                         some numerical models. The solar eclipse of October 14, 2023 was a 
                         partial solar eclipse that covered from North America, Central 
                         America and even northern part of South America. Prior to this 
                         event, predictions were made of the impact on the ionosphere 
                         during this eclipse. For this, the SUPIM (Sheffield University 
                         Plasmasphere-Ionosphere Model) was used: a numerical model that 
                         solves the coupled equations of continuity, momentum and energy 
                         dependent on time, along the magnetic field lines, and which has 
                         been updated and adapted by the Instituto Nacional de Pesquisas 
                         Espaciais (SUPIM-INPE). Particularly, in the case of predictions 
                         during solar eclipses, some adjustments have been made to the 
                         solar radiation according to the geometry of each solar eclipse. 
                         The objective of this work is to evaluate that prediction using 
                         the measurements available from some ionospheric stations that 
                         were covered during the eclipse. Modeling these phenomena helps us 
                         better understand the ionospheric impact and its consequences on 
                         communication and navigation systems.",
  conference-location = "Monterrey, Mexico",
      conference-year = "08-12 Apr. 2024",
             language = "en",
        urlaccessdate = "29 jun. 2024"
}