@TechReport{GonzalezGonzJard:1983:TrEnVe,
               author = "Gonzalez, Al{\'{\i}}cia Luisa Clua de and Gonzalez-Alarcon, 
                         Walter Dem{\'e}trio and Jardim, Maria Virg{\'{\i}}nia Alves",
                title = "Transfer{\^e}ncia de energia do vento solar {\`a} magnetosfera 
                         terrestre devido {\`a} jun{\c{c}}{\~a}o magn{\'e}tica na 
                         magnetopausa",
          institution = "Instituto Nacional de Pesquisas Espaciais",
                 year = "1983",
                 type = "RPQ",
               number = "INPE-2848-RPE/439",
              address = "S{\~a}o Jos{\'e} dos Campos",
             keywords = "reconex{\~a}o magn{\'e}tica, vento solar, magnetosfera.",
             abstract = "Algumas express{\~o}es gerais para os campos el{\'e}tricos 
                         paralelo e de convec{\c{c}}{\~a}o, bem como para a 
                         transfer{\^e}ncia de energia, devido {\`a} reconex{\~a}o na 
                         magnetopausa, s{\~a}o derivadas usando um modelo de 
                         reconex{\~a}o no {"}nariz{"} da magneto pausa, que leva em conta 
                         a presen{\c{c}}a dos {"}clefts{"}. Para o caso de amplitudes 
                         iguais do campo geomagn{\'e}tico e da bainha magn{\'e}tica, a 
                         express{\~a}o para a pot{\^e}ncia dissipada pelo campo 
                         el{\'e}trico de convec{\c{c}}{\~a}o se reduz ao par{\^a}metro 
                         de subtempestade E amplamente discutido na literatura atual. Este 
                         resultado sugere que a reconex{\~a}o na magnetopausa {\'e} 
                         definida no {"}nariz{"} com urna linha de reconet{\~a}o 
                         inclinada, mas que o campo el{\'e}trico de convec{\c{c}}{\~a}o 
                         est{\'a} relacionado somente com a componente {"}dawn-dusk{"} do 
                         campo el{\'e}trico de reconex{\~a}o, como definido em altas 
                         latitudes ({"}clefts{"}). ABSTRACT: An expression for the energy 
                         transfer due to magnetopause reconnection, as well as related 
                         expressions for the convection and parallel electric fields, are 
                         presented. These expression are derived from a reconnection model 
                         centered at the magnetopause nose, and that considers the presence 
                         of the clefts. The expression for the convection-electric 
                         field-related energy transfer reduces to the substorm parameter E 
                         for the special case of equal magnetosheath and geomagnetic field 
                         amplitudes. This result suggests that the reconnection electric 
                         field is transmitted along a tilted reconnection line, but that 
                         the convection field is only related to the {"}dawn to dusk{"} 
                         component of the reconnection-electric field.",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
           copyholder = "SID/SCD",
                label = "2393",
             language = "pt",
                pages = "23",
                  ibi = "6qtX3pFwXQZ3r59YCT/GTznq",
                  url = "http://urlib.net/ibi/6qtX3pFwXQZ3r59YCT/GTznq",
           targetfile = "publicacao.pdf",
        urlaccessdate = "29 jun. 2024"
}