@Article{CardosoGonSibKuzKog:2013:MaReIn,
               author = "Cardoso, Flavia R. and Gonzalez, Walter Demetrio and Sibeck, D. G. 
                         and Kuznetsova, M. and Koga, D.",
          affiliation = "EEL, USP-Escola de Engenharia de Lorena, Universidade de S{\~a}o 
                         Paulo, Lorena, S{\~a}o Paulo, Brazil; INPE, Instituto Nacional de 
                         Pesquisas Espaciais, S{\~a}o Jos{\'e} dos Campos, S{\~a}o 
                         Paulo, Brazil and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and NASA Goddard Space Flight Center, Greenbelt, MD, 
                         United States and NASA Goddard Space Flight Center, Greenbelt, MD, 
                         United States and INPE, Instituto Nacional de Pesquisas Espaciais, 
                         S{\~a}o Jos{\'e} dos Campos, S{\~a}o Paulo, Brazil",
                title = "Magnetopause reconnection and interlinked flux tubes",
              journal = "Annales Geophysicae",
                 year = "2013",
               volume = "31",
               number = "10",
                pages = "1853--1866",
             keywords = "magnetopause, magnetohydrodynamics, interplanetary magnetic 
                         field.",
             abstract = "Magnetic reconnection can be a continuous or a transient process. 
                         Global magnetohydrodynamics (MHD) simulations are important tools 
                         to understand the relevant magnetic reconnection mechanisms and 
                         the resulting magnetic structures. We have studied magnetopause 
                         reconnection using a global 3-D MHD simulation in which the 
                         interplanetary magnetic field (IMF) has been set to large positive 
                         By and large negative Bz components, i.e., a south-duskward 
                         direction. Flux tubes have been observed even during these 
                         constant solar wind conditions. We have focused on the interlinked 
                         flux tubes event resulting from time-dependent, patchy and 
                         multiple reconnection. At the event onset, two reconnection modes 
                         seem to occur simultaneously: a timedependent, patchy and multiple 
                         reconnection for the subsolar region; and, a steady and 
                         large-scale reconnection for the regions far from the subsolar 
                         site.",
                  doi = "10.5194/angeo-31-1853-2013",
                  url = "http://dx.doi.org/10.5194/angeo-31-1853-2013",
                 issn = "0992-7689",
                label = "scopus 2013-11",
             language = "en",
           targetfile = "angeo-31-1853-2013.pdf",
        urlaccessdate = "04 maio 2024"
}