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@InProceedings{VieiraDSGSCASJ:2019:StGaSo,
               author = "Vieira, Lu{\'{\i}}s 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 = "Status of the Galileo Solar Space Telescope Mission (GSST) 
                         proposal",
                 year = "2019",
         organization = "AGU Fall Meeting",
             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 the proposal submitted to the INPE's Steering Committee. 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 Earth's 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 Sun's influence on Earth's Climate; and, (3) 
                         Contribute to the understanding of the Sun's impact on the 
                         Geospace.",
  conference-location = "San Francisco, CA",
      conference-year = "09-13 dec.",
             language = "en",
           targetfile = "vieira_status.pdf",
        urlaccessdate = "14 abr. 2021"
}


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