@Article{SilbergleitGonz:2009:RiCuSp,
               author = "Silbergleit, Virginia M. and Gonzalez Alarcon, Alicia Luisa 
                         Cl{\'u}a de",
          affiliation = "{Universidad Nacional de Buenos Aires} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Ring current space time inhomogeneities observed during intense 
                         geomagnetic storms",
              journal = "Acta Geodaetica et Geophysica Hungarica",
                 year = "2009",
               volume = "44",
               number = "2",
                pages = "149--156",
                month = "June",
             keywords = "auroral activity, interplanetary magnetic field, IMF, magnetic 
                         storm, ring current, velocity of solar wind.",
             abstract = "The behavior of the horizontal component of the magnetic field 
                         obtained by ground magnetometers for three intense magnetic storms 
                         that happened during the occurrence of continual auroral activity 
                         (HILDCAAs) was studied through a UT-LT analysis. The considered 
                         storm periods were August 2628, 1998, October 2123, 1999 and April 
                         68, 2000. Five minute resolution data were taken from six magnetic 
                         observatories, with approximately uniform longitudinal 
                         distribution. The results were compared with some interplanetary 
                         parameters such as velocity of solar wind, south component of 
                         interplanetary magnetic field.",
                  doi = "10.1556/AGeod.44.2009.2.1",
                  url = "http://dx.doi.org/10.1556/AGeod.44.2009.2.1",
                label = "lattes: 7209946672198332 2 SilbergleitGonz:2009:RiCuSp",
             language = "en",
        urlaccessdate = "15 jun. 2024"
}