@InProceedings{CandidoSBCCKWSCL:2019:RoSoWi,
               author = "Candido, Cl{\'a}udia Maria Nicoli and Shi, Jiankui and 
                         Becker-Gueder, F{\'a}bio and Correia, Em{\'{\i}}lia and 
                         Cecatto, Jos{\'e} Roberto and Klausner, Virg{\'{\i}}nia and 
                         Wang, Chi and Santos, Stella Pires de Moraes and Chingaranki, 
                         Frank and Liu, Zhengkuan",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {NSSC/Chinese Academy of Sciences} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} 
                         and {Chinese Academy of Sciences} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Chinese Academy of Sciences}",
                title = "The role of the solar wind on the low-latitude ionosphere during 
                         the descending phase of solar cycle 24",
                 year = "2019",
         organization = "AGU Fall Meeting",
             abstract = "The descending phase of the solar cycle is characterized by the 
                         increased occurrence rate of solar coronal holes which emanated 
                         high-speed solar wind streams to the interplanetary space. As they 
                         propagate in the space they interact with the preceding slow solar 
                         wind and form large structures called interaction region or 
                         corotating interaction regions. Although these interplanetary 
                         structures do not cause intense geomagnetic storms, they are 
                         responsible by a variety of phenomena such as: long duration 
                         auroral activity, referred as HILDCAAs, electric field-driven 
                         effects, such as prompt penetration or disturbance dynamo, 
                         particle precipitation, ionospheric storms/neutral composition 
                         changes, disturbed equatorward wind system and others. In order to 
                         understand the influence of the solar wind on the ionospheric 
                         variability, we study the relationship between the distinct 
                         features of the coronal holes, solar wind, interplanetary and 
                         geomagnetic indices and parameters such as, solar wind speed, Vsw, 
                         interplanetary magnetic field, B, auroral electrojet index, AE, 
                         symmetric ring current, SymH, and the ionospheric parameters. 
                         After that, we analyzed the ionospheric response in the distinct 
                         phases of the storms, which is highly variable especially due to 
                         the high Alfvenicity of the magnetic field and to the extended 
                         recovery phase of the storms. For the purpose of this study, we 
                         used instruments including GNSS receivers, ionosondes, 
                         magnetometers, and other ground-based systems. This study may be 
                         useful for ionospheric modelling and Space Weather forecast 
                         models.",
  conference-location = "San Francisco, CA",
      conference-year = "09-13 dec.",
             language = "en",
           targetfile = "candido_role.pdf",
        urlaccessdate = "19 abr. 2024"
}