@InProceedings{SavianSSADVMGS:2004:AnInSt,
               author = "Savian, Jairo Francisco and Silva, Marlos Rockenbah da and 
                         Signori, Marcos Roberto and Andrioli, V{\^a}nia F{\'a}tima and 
                         Dal Lago, Alisson and Vieira, Luiz Eduardo Antunes and Munakata, 
                         K. and Gonzalez Alarcon, Walter Dem{\'e}trio and Schuch, Nelson 
                         Jorge",
          affiliation = "{Universidade Federal de Santa Maria (UFSM)} and {Universidade 
                         Federal de Santa Maria (UFSM)} and {Universidade Federal de Santa 
                         Maria (UFSM)} and {Universidade Federal de Santa Maria (UFSM)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Analysis of interplanetary structures associated with cosmic ray 
                         precursory anisotropies and intense geomagnetic storms",
            booktitle = "Anais...",
                 year = "2004",
         organization = "Scientific Assembly of COSPAR, (37Th).",
            publisher = "INPE",
             abstract = "Throughout the 11 year solar cycle a number of energetic phenomena 
                         such as {"}flares{"} and coronal mass ejections (CME) give rise at 
                         earth to the so-called magnetic storms. These storms are 
                         characterized by a decrease in the H component of terrestrial 
                         magnetic field, lasting some dozens of hours. They are associated 
                         to interplanetary structures whose interplanetary magnetic field 
                         component in the Z direction (Bz) is southward, i.e., antiparalell 
                         to the earth's magnetic field direction. Thus, the interplanetary 
                         magnetic field interconnects with the geomagnetic field causing 
                         energy to be transported inwards. Some of these structures are 
                         associated with precursory anisotropy observed in ground cosmic 
                         ray data (muons). The objective of this work is to use a set of 
                         intense geomagnetic storm events (Dst.",
  conference-location = "Paris, France",
      conference-year = "18-25 july",
                label = "self-archiving-INPE-MCTIC-GOV-BR",
             language = "en",
        urlaccessdate = "09 maio 2024"
}