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@Article{EvangelistaMiraMendDomi:2019:SiInNo,
               author = "Evangelista, Edgard de Freitas Diniz and Miranda, Oswaldo Duarte 
                         and Mendes, Odim and Domingues, Margarete Oliveira",
          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)}",
                title = "Simulating the Interaction of a Non-magnetized Planet with the 
                         Stellar Wind Produced by a Sun-like Star Using the FLASH Code",
              journal = "Brazilian Journal of Physics",
                 year = "2019",
               volume = "49",
               number = "5",
                pages = "678--692",
                month = "Oct.",
             keywords = "Stellar winds  Magnetohydrodynamics  FLASH code  Numerical 
                         methods.",
             abstract = "The study of the interaction between solid objects and 
                         magnetohydrodynamic (MHD) fluids is of great importance in physics 
                         as a consequence of the significant phenomena generated, such as 
                         planets interacting with stellar wind produced by their host 
                         stars. There are several computational tools created to simulate 
                         hydrodynamic and MHD fluids, such as the FLASH code. In this code, 
                         there is a feature which permits the placement of rigid bodies in 
                         the domain to be simulated. However, it is available and tested 
                         for pure hydrodynamic cases only. Our aim here is to adapt the 
                         existing resources of FLASH to enable the placement of a rigid 
                         body in MHD scenarios and, with such a scheme, to produce the 
                         simulation of a non-magnetized planet interacting with the stellar 
                         wind produced by a sun-like star. Besides, we consider that the 
                         planet has no significant atmosphere. We focus our analysis on the 
                         patterns of the density, magnetic field, and velocity around the 
                         planet, as well as the influence of viscosity on such patterns. At 
                         last, an improved methodological approach is available to other 
                         interested users.",
                  doi = "10.1007/s13538-019-00689-y",
                  url = "http://dx.doi.org/10.1007/s13538-019-00689-y",
                 issn = "0103-9733",
             language = "en",
           targetfile = "evangelista_simulating.pdf",
        urlaccessdate = "17 abr. 2021"
}


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