@Article{LuiGonz:2013:ReSoWi,
               author = "Lui, A. T. Y. and Gonzalez, Walter Demetrio",
          affiliation = "JHU/APL, Laurel, MD 20723-6099, United States and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "Reconstruction of solar wind features that caused a super 
                         geomagnetic storm",
              journal = "AIP Conference Proceedings",
                 year = "2013",
               volume = "1539",
                pages = "406--409",
                month = "June",
                 note = "SOLAR WIND 13: Proceedings of the Thirteenth International Solar 
                         Wind Conference, 17–22 June 2012, Big Island, Hawaii",
             keywords = "superstorm, magnetic cloud, Grad-Shafranov reconstruction.",
             abstract = "A superstorm with Dst < -300 nT can cause major space 
                         disturbances. We examine one on March 31, 2001 that has the 
                         minimum Dst of -387 nT and obtain two-dimensional maps in pressure 
                         and magnetic field of the sheath region and a magnetic cloud 
                         behind it. Both the sheath and the magnetic cloud play a role in 
                         building the storm strength. Several properties of the magnetic 
                         cloud are inferred, including an estimated total magnetic flux of 
                         <6.5×10 12 Wb.",
     alternatejournal = "Big Island, HI",
                  doi = "10.1063/1.4811071",
                  url = "http://dx.doi.org/10.1063/1.4811071",
                 isbn = "9780735411630",
                 issn = "0094-243X",
                label = "scopus 2013-11",
             language = "en",
        urlaccessdate = "15 jun. 2024"
}