@InProceedings{SilvaSMSAVADRCWMLJIZ:2022:HiElFl,
               author = "Silva, Ligia Alves da and Shi, Jiankui and Marchezi, Jos{\'e} 
                         Paulo and Sibeck, David and Alves, Livia Ribeiro and Vieira, 
                         Lu{\'{\i}}s Eduardo Antunes and Agapitov, Oleksiy and Deggeroni, 
                         Vinicius and Resende, Laysa Cristina Ara{\'u}jo and Costa, 
                         Joaquim Eduardo Rezende and Wang, Chi and Moro, Juliano and Li, 
                         Hui and Jauer, Paulo Ricardo and Inostroza, Ana Maria and 
                         Zhengkuan, Liu",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Chinese 
                         Academy of Sciences (CAS)} and {Chinese Academy of Sciences (CAS)} 
                         and {NASA GSFC} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {UC Berkeley} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Chinese 
                         Academy of Sciences (CAS)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Chinese Academy of Sciences (CAS)}",
                title = "High-energy electron flux enhancement pattern in the outer 
                         radiation belt in response to the coronal mass ejections",
                 year = "2022",
         organization = "COSPAR Scientific Assembly, 44.",
             abstract = "We consider the high-energy electron flux enhancements that occur 
                         in the outer radiation belt in response to Interplanetary Coronal 
                         Mass Ejections (ICMEs). We selected ten events during the Van 
                         Allen Probes era in which the high-energy electron flux 
                         enhancements start at L-shells below 3.8. Although the physical 
                         processes responsible for high-energy electron flux enhancements 
                         in the outer radiation belt are known to be associated with the 
                         dynamics of the incident solar wind structures and interplanetary 
                         transients, there are still several open questions. This work 
                         seeks to identify the sequence of ideal physical processes needed 
                         for highenergy electron flux enhancements that occur under the 
                         influence of the ICMEs via an epoch analysis applied to the 
                         interplanetary medium parameters that define ICMEs. Additionally, 
                         the dynamic mechanisms driven by both whistler-mode chorus and 
                         ultra low-frequency waves will be discussed individually and 
                         through epoch analyses to identify the role of these waves in the 
                         electron flux enhancement pattern. Thereby, the results of this 
                         work may offer support models for the radiation belts within the 
                         inner magnetosphere.",
  conference-location = "Athens, Greece",
      conference-year = "16-24 July 2022",
             language = "en",
           targetfile = "PRBEM.3-0016-22-oral.pdf",
        urlaccessdate = "20 maio 2024"
}