@Article{EcherEcDoMeSeGo:2021:WaAnLo,
               author = "Echer, Mariza Pereira de Souza and Echer, Ezequiel and Domingues, 
                         Margarete Oliveira and Mendes, Odim and Seo, Rodrigo Takeshi and 
                         Gonzalez Alarcon, Walter Dem{\'e}trio",
          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)}",
                title = "Wavelet analysis of low frequency magnetic field fluctuations in 
                         the Jupiter's magnetotail",
              journal = "Advances in Space Research",
                 year = "2021",
               volume = "68",
               number = "1",
                pages = "246--258",
                month = "jULY",
             keywords = "Jupiter's magnetosphere, Jupiter's magnetotail, Low frequency 
                         oscillations, Continuous wavelet transform.",
             abstract = "Jupiter's magnetospheric processes are strongly influenced by the 
                         planet fast rotation and by its internal plasma sources. As a 
                         consequence, the 10-h rotation period signal is dominant on many 
                         datasets. In this work, in order to study low frequency magnetic 
                         fluctuations in the Jupiter's magnetotail, the continuous wavelet 
                         transform (CWT) analysis is employed to investigate the magnetic 
                         field vector data during six orbits of Galileo spacecraft. Besides 
                         the near 10-h Jovian rotation period, the major periods found in 
                         this study are 5-h, most likely due to transient disturbances in 
                         Jupiter's magnetosphere, and from 1.5 to 3.5 days, possibly 
                         related to global reconfiguration in the magnetosphere.These 
                         periodicities may also be related to the mass-loading from the 
                         moon Io and to possible modulation by the solar wind. Furthermore, 
                         long periods have been also found from 5 to 35 days. The method 
                         presented in this study could be very useful for application in 
                         other datasets of planetary magnetospheres.",
                  doi = "10.1016/j.asr.2021.03.003",
                  url = "http://dx.doi.org/10.1016/j.asr.2021.03.003",
                 issn = "0273-1177 and 1879-1948",
             language = "en",
           targetfile = "echer_wavelet.pdf",
        urlaccessdate = "09 maio 2024"
}