@InProceedings{MarcheziAlveSilv:2018:BeULMe,
               author = "Marchezi, Jos{\'e} Paulo and Alves, Livia Ribeiro and Silva, 
                         Ligia Alves da",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Behavior of the ULF mean power spectral density on the electron 
                         flux variation related to CME and HSS structures during the Van 
                         Allen Probes era",
                 year = "2018",
         organization = "Latin American Conference on Space Geophysics, 11. (COLAGE)",
             abstract = "The ULF frequency range are know to play a significant role on the 
                         energy changes of the Van Allenīs outer radiation belt electron 
                         flux, violating the third adiabatic invariant, through a resonant 
                         interaction. The main mechanism involved is the radial diffusion, 
                         it is an stochastic process that take account the wave and the 
                         particle drift frequencies. There are some proposed models to 
                         explain the ULF-particle interaction deriving the radial diffusion 
                         coefficients. All the models consider the polarization modes of 
                         the ULF waves on the efficiency of the interaction. The 
                         contribution of the fluctuation of the magnetic and electric field 
                         are computed taking account the power spectrum density (PSD) of 
                         the signal. This work aims to estimate the behavior of the 
                         integrated ULF wave PSD amplitude, in the frequency range of the 
                         Pc3 and Pc5 geomagnetic pulsation on the magnetic field data 
                         recorded ground based stations from the Churchill line disposition 
                         of the Canadian Array for Realtime Investigations of Magnetic 
                         Activity (CARISMA) magnetometer network, for all the cases that 
                         have an increase on the 2.10 MeV electrons recorded by the 
                         Relativistic Electron Proton Telescope (REPT) instrument, on board 
                         of the Van Allen Probes, related to Coronal Mass Ejection (CME) 
                         and High Speed Streams (HSS) events, during the October 2012 to 
                         December 2016 period. This arrangement allows the verification of 
                         the PSD according to the radial distance in the magnetosphere, 
                         covering all the external radiation belt region.",
  conference-location = "Buenos Aires, Argentina",
      conference-year = "16-20 abr.",
             language = "en",
        urlaccessdate = "28 abr. 2024"
}