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@InProceedings{DalLagoBragMesqMend:2017:PrICPr,
               author = "Dal Lago, Alisson and Braga, Carlos Roberto and Mesquita, Amanda 
                         Lucia and Mendon{\c{c}}a, Rafael Rodrigues Souza de",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)}",
                title = "Predicting ICME properties at 1AU",
            booktitle = "Proceedings...",
                 year = "2017",
         organization = "AGU Fall Meeting",
             abstract = "Coronal mass ejections (CMEs) are among the main origins of 
                         geomagnetic disturbances. They change the properties of the 
                         near-earth interplanetary medium, enhancing some key parameters, 
                         such as the southward interplanetary magnetic field and the solar 
                         wind speed. Both quantities are known to be related to the energy 
                         transfer from the solar wind to the Earths magnetosphere via the 
                         magnetic reconnection process. Many attempts have been made to 
                         predict the magnetic filed and the solar wind speed from 
                         coronagraph observations. However, we still have much to learn 
                         about the dynamic evolution of ICMEs as they propagate through the 
                         interplanetary space. Increased observation capability is probably 
                         needed. Among the several attempts to establish correlations 
                         between CME and ICME properties, it was found that the average CME 
                         propagation speed to 1AU is highly correlated to the ICME peak 
                         speed (Dal Lago et al, 2004). In this work, we present an extended 
                         study of such correlation, which confirms the results found in our 
                         previous study. Some suggestions on how to use this kind of 
                         results for space weather estimates are explored.",
  conference-location = "New Orleans",
      conference-year = "11-15 Dec.",
             language = "en",
        urlaccessdate = "25 nov. 2020"
}


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