@Article{JauerWESSMAADLLHVGDMC:2022:EnCoUl,
               author = "Jauer, Paulo Ricardo and Wang, C. and Echer, Ezequiel and Souza, 
                         Vitor Moura Cardoso e Silva and Silva, Ligia Alves da and 
                         Marchezi, Jos{\'e} Paulo and Alves, Livia Ribeiro and Alves, 
                         Maria Virg{\'{\i}}nia and Douglas, S. and Loesch, C. and Liu, Z. 
                         and Hui, L. and Vieira, Lu{\'{\i}}s Eduardo Antunes and Gonzalez 
                         Alarcon, Walter Demetrio and Denardini, Clezio Marcos and 
                         Medeiros, Cl{\'a}udia and Costa, Joaquim Eduardo Rezende",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {State Key 
                         Laboratory of Space Weather (NSSC)} 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 {State Key Laboratory 
                         of Space Weather} and {Institute of Higher Education of 
                         Bras{\'{\i}}lia} and {State Key Laboratory of Space Weather} and 
                         {State Key Laboratory of Space Weather} 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 = "Global Modeling of the Inner Magnetosphere Under the Influence of 
                         a Magnetic Cloud Associated With an Interplanetary Coronal Mass 
                         Ejection: Energy Conversion and Ultra-Low Frequency Wave 
                         Activity",
              journal = "Journal of Geophysical Research: Space Physics",
                 year = "2022",
               volume = "127",
               number = "10",
                pages = "e2022JA030615",
                month = "Oct.",
             keywords = "energy conversion, MHD simulation, ULF waves, magnetic cloud, 
                         magnetospheric activity.",
             abstract = "The interaction and response of the magnetic cloud-type structure 
                         with Earth's magnetosphere were modeled by the SWMF/BATS-R-US 
                         code. The conversion of magnetic (E-m), kinetic (E-k), and 
                         internal (E-i) energies was analyzed as well as the wave power 
                         integrated in the ultra-low frequency (ULF) range of the poloidal 
                         (E-phi) and toroidal (E-r) electric field components in the 
                         equatorial region of the magnetosphere, in seven 2-hr long 
                         intervals, namely, I1 through I7. The intensity of energy 
                         conversion and wave activity for I1 and I7 intervals was 
                         negligible. The energy conversion started in the I2 interval and 
                         extended to the I3, I4, and I5 intervals. The power of the E-phi 
                         and E-r components in the dayside and nightside regions is clearly 
                         observed. The I4 corresponds to interplanetary magnetic field 
                         (IMF) B-z mostly southward and the I5 has similar amplitudes of 
                         the B-z and B-y components, corresponding to the period of the 
                         high geomagnetic activity. The conversion rate for the I4 and I5 
                         was similar, however, the integrated power spectral density (IPSD) 
                         of the E-phi and E-r components is more intense in I5. During the 
                         I6 interval, with predominant IMF B-y, the energy conversion rate 
                         is intensified mostly for inner radial distances R R-E, and the 
                         E-k component becomes close to zero for outer regions. The energy 
                         conversion regions are located spatially close to or overlapping 
                         with regions where the IPSD in the ULF range is intensified. The 
                         energy conversion in the inner magnetosphere occurred 
                         preferentially between E-m and E-i, with the E-k energy component 
                         always present but with lower intensities.",
                  doi = "10.1029/2022JA030615",
                  url = "http://dx.doi.org/10.1029/2022JA030615",
                 issn = "2169-9402",
             language = "en",
           targetfile = "JGR Space Physics - 2022 - Jauer - Global Modeling of the Inner 
                         Magnetosphere Under the Influence of a Magnetic Cloud.pdf",
        urlaccessdate = "03 maio 2024"
}