@InProceedings{EcherGonz:2006:SoCyDi,
               author = "Echer, Ezequiel and Gonzalez, Walter Dem{\'e}trio",
          affiliation = "Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de 
                         Geof{\'{\i}}sica Espacial (INPE.DGE) and Instituto Nacional de 
                         Pesquisas Espaciais, Divis{\~a}o de Geof{\'{\i}}sica Espacial 
                         (INPE.DGE)",
                title = "On the solar cycle distribution of geomagnetic storms",
            booktitle = "Proceedings...",
                 year = "2006",
         organization = "European Geosciences Union (EGU) General Assembly.",
             abstract = "We present a study on the solar cycle distribution of geomagnetic 
                         storms.We have determined the number of storms per year within 
                         several Dst ranges, from 1957 to 2002. Moderate storms have showed 
                         a peak near solar cycle maxima. As the storm intensity rises, 
                         however, a dual peak distribution starts to appear. The strongest 
                         storm distributions have peaks just before solar maximum and 
                         around the descending solar cycle phase. There seems to be a trend 
                         for weaker cycles to have a lower number of storms, of any 
                         intensity. Very intense magnetic storms can occur more frequently 
                         around solar maximum and declining phases. The variation of the 
                         southward component of the interplanetary magnetic field with 
                         solar cycle epoch is also investigated in this work.",
  conference-location = "Vienna, Austria",
      conference-year = "2006-04-02",
             language = "en",
        urlaccessdate = "16 jun. 2024"
}