@InProceedings{VieiraDSGSCASJ:2021:INCoIn,
               author = "Vieira, Luis Eduardo Antunes and Dal Lago, Alisson and Silva, 
                         Marlos Rockenbach da and Guarnieri, Fernando Lu{\'{\i}}s and 
                         Silva, Ligia Alves da and Carlesso, Franciele and Alves, Livia 
                         Ribeiro and Souza, Vitor Moura Cardoso e Silva and Jauer, Paulo 
                         Ricardo",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "INGV contribution to international Space Weather initiatives",
                 year = "2021",
         organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e 
                         Aeronomia, 8. (SBGEA)",
             abstract = "The Galileo Solar Space Telescope (GSST) is a cornerstone mission 
                         to provide accurate measurements of the magnetic field in the 
                         photosphere and outer layers of the solar atmosphere to be 
                         proposed to the Brazilian Space Agency (AEB) within the 
                         international effort to understand of the evolution of the 
                         Heliosphere. The solar electromagnetic and corpuscular emissions 
                         are strongly modulated by the evolution of the magnetic structure 
                         of the solar atmosphere. The solar magnetism is driven by the 
                         energy transport from the inner layers of the Sun to its 
                         atmosphere. Although systematic observations since the invention 
                         of the telescope have revealed several features related to the 
                         evolution of solar activity, there is not a complete explanation 
                         of the physical processes that lead to solar activity cyclic 
                         variability and its long-term changes. Here we describe the status 
                         of missions Phase 0/A. The underlying basic questions to be 
                         addressed by the GSST mission are: What are the fundamental 
                         physical/plasma processes at work in the Sun? How does the solar 
                         dynamo work? What is the relative contribution of different 
                         physical processes that lead to the heating of the outer layers 
                         (Chromosphere to Corona)? What are the effects of the magnetic 
                         structure of the outer layers of the Sun on the evolution of the 
                         Earths highly coupled atmosphere-ocean system? What is the 
                         response of the magnetic field and energetic particles in the 
                         vicinity of our planet, i.e. the Earths inner magnetosphere 
                         region, due to different solar wind structures? Taking into 
                         account these open scientific questions, the Galileo Solar Space 
                         Telescope proposed mission is to perform solar observations in 
                         high spatial and temporal resolution to characterize the evolution 
                         of the magnetic structure of the photosphere, chromosphere, 
                         transition region, and corona and its impact on the Geospace. 
                         Specifically, the mission has three main objectives: (1) 
                         Contribute to the understanding of the evolution of the magnetic 
                         structure of the Sun; (2) Contribute to the understanding of the 
                         Suns influence on Earths Climate; and, (3) Contribute to the 
                         understanding of the Suns impact on the Geospace. This 
                         contribution is an update of the previous version presented at the 
                         AGU Fall Meeting 2019.",
  conference-location = "Online",
      conference-year = "22-26 mar.",
             language = "en",
        urlaccessdate = "09 maio 2024"
}