@InProceedings{LucasGEGDVSS:2007:CoInPa,
               author = "Lucas, Aline de and Gonzalez Alarcon, Walter Dem{\'e}trio and 
                         Echer, Ezequiel and Guarnieri, Fernando Lu{\'{\i}}s and Dal 
                         Lago, Alisson and Vieira, L. E. A. and Silva, Marlos Rockenbach da 
                         and Saraiva, A. C. V.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and UNIVAP and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and UNIVAP and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Universidade Presbiteriana 
                         Mackenzie}",
                title = "A comparison of interplanetary parameters and geomagnetic indices 
                         during intense and super intense magnetic storms",
            booktitle = "Proceedings...",
                 year = "2007",
         organization = "European Geosciences Union General Assembly 2007. (EGU 
                         Assembly).",
             abstract = "Geomagnetic storms are great disturbances on the magnetic field of 
                         the Earth, which are conventionally measured by the Dst 
                         geomagnetic index. Of great importance to space weather 
                         environment is the development of intense (-250 < Dst < -100 nT) 
                         and very intense magnetic storms (Dst < -250 nT). One point of 
                         current research is the study of the interplanetary causes and 
                         consequent magnetospheric response during these two classes of 
                         storm. For each storm class, it have been determined the 
                         interplanetary parameters such as Ey, Bz, and the solar wind ram 
                         pressure, PSW, and geomagnetic indices, Dst/Sym, Asy, AE, and Kp. 
                         The main goal of this study is to distinguish the interplanetary 
                         causes and the magnetospheric responses of intense and very 
                         intense magnetic storms. Besides, a criterion which characterizes 
                         the space weather phenomena during different disturbed levels is 
                         suggested.",
  conference-location = "Vienna, Austria",
      conference-year = "15-20 Apr.",
             language = "en",
        urlaccessdate = "12 maio 2024"
}