@InProceedings{MarcheziDASSDSJVCDAWLL:2022:StAnVa,
               author = "Marchezi, Jos{\'e} Paulo and Dai, Lei and Alves, Livia Ribeiro 
                         and Silva, Ligia Alves da and Sibeck, David G. and Dal Lago, 
                         Alisson and Souza, Vitor Moura Cardoso e Silva and Jauer, Paulo 
                         Ricardo and Vieira, Lu{\'{\i}}s Eduardo Antunes and Cardoso, 
                         Fl{\'a}via Regina and Deggeroni, Vinicius and Alves, Maria 
                         Virg{\'{\i}}nia and Wang, Chi and Li, Hui and Lui, Zhengkuan",
          affiliation = "{Chinese Academy of Sciences} and {Center for Space Science and 
                         Applied Research (CSSAR)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Chinese Academy of Sciences} and NASA/GSFC 
                         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 
                         CSSAR and {NSSC National Space Science Center} and {NSSC National 
                         Space Science Center}",
                title = "Electron flux variability and Ultra-low frequency wave activity in 
                         the outer radiation belt under the influence of Interplanetary 
                         Coronal Mass Ejections and High-Speed solar wind Streams: A 
                         statistical analysis from the Van Allen Probes Era",
                 year = "2022",
         organization = "AGU Fall Meeting",
            publisher = "AGU",
             abstract = "The ultra-low frequency (ULF) waves can stochastically accelerate 
                         radiation belt electrons. Radial diffusion is a well-established 
                         mechanism that can enhance or reduce the electron population in 
                         combination with other processes. Using data from the Van Allen 
                         Probes, we investigated the response of the 2.10 MeV energy 
                         electrons and ULF waves to two types of solar wind structures 
                         interacting with Earth's magnetosphere, namely, interplanetary 
                         coronal mass ejections (ICMEs) and High-Speed solar wind streams 
                         (HSS). We use measured electron differential flux and ULF waves in 
                         the Pc4--Pc5 frequency range from October 2012 to May 2019. We 
                         examine 155 events with changes in the outer radiation belt 
                         electron differential flux. Results considering all ICMEs and HSSs 
                         during the Van Allen Probes era show that for both solar wind 
                         structures, solar wind interplanetary magnetic field Bz, solar 
                         wind proton density, and speed are related to the outer radiation 
                         belt relativistic electrons' response. The persistent ULF power is 
                         present during enhancement cases, while for reduction, the ULF 
                         waves power is concentrated at the initial reduction on the outer 
                         radiation belt electron flux.",
  conference-location = "Chicago, IL",
      conference-year = "12-16 Dec. 2022",
        urlaccessdate = "27 abr. 2024"
}