@Article{González-AlarconTsurGonz:2002:GeStCo,
               author = "Gonz{\'a}lez-Alarcon, Walter Dem{\'e}trio and Tsurutani, Bruce 
                         T. and Gonz{\'a}lez-Alarcon, Alicia Luiza Cl{\'u}a de",
          affiliation = "Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de 
                         Geof{\'{\i}}sica Espacial and UBA, Fac Ingn, Buenos Aires, DF, 
                         Argentina and CALTECH, Jet Prop Lab, Pasadena, SA",
                title = "Geomagnetic storms contrasted during solar maximum and near solar 
                         minimum",
              journal = "Advances in Space Research",
                 year = "2002",
               volume = "30",
               number = "10",
                pages = "2301--2304",
             keywords = "magnetic storms, interplanetary, origin.",
             abstract = "Although considerable attention has been focused on CMEs/magnetic 
                         clouds and geomagnetic activity during solar maximum, very little 
                         effort has been expended towards understanding the effects of 
                         proto CIRs (Corotating Interaction Regions) during the descending 
                         phase of the solar cycle. We show that the three phases of 
                         magnetic storms (initial, main and recovery) associated to proto 
                         CIRs are considerably different than those during solar maximum. 
                         We also indicate that auroral activity can be significantly higher 
                         during the descending phase than during solar maximum.",
           copyholder = "SID/SCD",
                 issn = "0273-1177",
             language = "en",
           targetfile = "1-s2.0-S0273117702802526-main.pdf",
        urlaccessdate = "03 maio 2024"
}