@InProceedings{AlvesSSJVSSD:2015:OuRaBe,
               author = "Alves, Livia Ribeiro and Silva, L{\'{\i}}gia Alves da and Souza, 
                         Vitor Moura Cardoso e Silva and Jauer, Paulo Ricardo and Vieira, 
                         Luis Eduardo Antunes and Silveira, Marcos Vin{\'{\i}}cius Dias 
                         and Silva, Marlos Rockenbach da and Dal Lago, Alisson",
          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)}",
                title = "Outer radiation belt dropout on September 12, 2014",
                 year = "2015",
         organization = "International Congress of the Brazilian Geophysical Society, 14.",
             abstract = "Solar wind variations and magnetospheric processes result in a 
                         dynamic electron population within the outer Van Allen radiation 
                         belt, where electron energies range from several 10s to several 
                         1000s KeV. Geomagnetic storms and various solar wind-magnetosphere 
                         interaction processes including convection cause either dramatic 
                         particle flux increase or decreases. Here we analyze the 
                         occurrence of a drop out of ~ 0.04 4.5 MeV electron fluxes 
                         measured by NASA's Van Allen Probes, during a magnetic 
                         cloud-driven geomagnetic storm which started at September 12, 
                         2014. The ~3-day storm left a steady low flux of outer belt 
                         energetic electrons that lasted for twelve days. At higher energy 
                         levels, electron fluxes decreased by ~1 orders of magnitude 
                         throughout the vast region from L* ~3 to 6.6. To describe the 
                         physical mechanism associated to the loss observed at L* higher 
                         than 4, it was simulated electron trajectory using TS95 and 
                         self-consistent BATS-RUS models of magnetic field during the 
                         shock, the results are consistent with the magnetopause 
                         shadowing.",
  conference-location = "Rio de Janeiro, RJ",
      conference-year = "3-6 Aug.",
        urlaccessdate = "19 abr. 2024"
}