@InProceedings{JauerWSAPMASLLGVDECD:2019:CoInRe,
               author = "Jauer, Paulo Ricardo and Wang, Chi and Souza, Vitor Moura Cardoso 
                         e Silva and Alves, Maria Virg{\'{\i}}nia and Paula, Marcelo 
                         Banik de and Marchezi, Jos{\'e} Paulo and Alves, Livia Ribeiro 
                         and Silva, L{\'{\i}}gia Alves da and Li, Hui and Liu, Zhengkuan 
                         and Gonzalez Alarcon, Walter Dem{\'e}trio and Vieira, 
                         Lu{\'{\i}}s Eduardo Antunes and Dal Lago, Alisson and Echer, 
                         Ezequiel and Medeiro and Costa, Joaquim Eduardo Rezende and 
                         Denardin, Clezio Marcos",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and CSSAR, CAS 
                         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 NSSC National Space Science Center, CAS and NSSC 
                         National Space Science Center, CAS 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 = "A Global Magnetohydrodynamic Simulation Study of Ultra-Low 
                         Frequency Waves Activity in the Inner Magnetosphere: Corotating 
                         Interaction Region + Alfv{\'e}nic Fluctuation",
                 year = "2019",
         organization = "AGU Fall Meeting",
             abstract = "comprised of a Corotating Interaction Region (CIR) followed by 
                         solar wind Alfv{\'e}nic fluctuations it is not straightforward to 
                         decisively say which solar wind parameters or which combinations 
                         thereof are most effective in causing disturbances in the inner 
                         magnetosphere, or how each part of the complex interplanetary 
                         structure influences the most the temporal evolution of the 
                         magnetosphere. Using global magnetohydrodynamic (MHD) simulations 
                         we perform a study which address some of these questions. Firstly, 
                         we use the magnetic field and plasma parameters of a real 
                         CIR+Alfv{\'e}nic fluctuations event as input to the 
                         SWMF/BATS-R-US code. The model outputs are used to calculate the 
                         convection electric field's power spectral density (PSD) 
                         integrated in the ultra-low frequency (ULF) waves frequency range 
                         in the equatorial, nightside magnetosphere region. Then, we 
                         separate the real event into its constituent parts by building up 
                         synthetic magnetic field and plasma profiles based on the physical 
                         parameters which characterize each of these parts. The MHD code is 
                         then fed with each new synthetic profile containing Alfv{\'e}nic 
                         fluctuations with two driving frequencies, namely 0.833 and 1.66 
                         mHz. Our preliminary results show that the toroidal electric field 
                         (Er) component fluctuations are related with both driving 
                         frequencies, specially at farther out locations near the flanks of 
                         the modeled magnetopause. The poloidal (Ef) component fluctuations 
                         do respond differently to the driving frequencies in terms of both 
                         spatial structure and integrated power intensities.",
  conference-location = "San Francisco, CA",
      conference-year = "09-13 dec.",
             language = "en",
           targetfile = "jauer_global.pdf",
        urlaccessdate = "27 abr. 2024"
}