Logo do repositório
  • English
  • Español
  • Português do Brasil
  • Entrar
    Novo usuário? Clique aqui para cadastrar. Esqueceu sua senha?
Logo do repositório
  • Comunidades e Coleções
  • Navegar
  • English
  • Español
  • Português do Brasil
  • Entrar
    Novo usuário? Clique aqui para cadastrar. Esqueceu sua senha?
  1. Início
  2. Pesquisar por Autor

Navegando por Autor "Bageston, Jose Valentin"

Agora exibindo 1 - 1 de 1
Resultados por página
Opções de Ordenação
  • Carregando...
    Imagem de Miniatura
    Item
    Study of height-spread sporadic-E layers observed in the South American Magnetic Anomaly
    (Frontiers) Moro, Juliano; Xu, Jiyao; Bageston, Jose Valentin; Silva, Ligia Alves da; Resende, Laysa Cristina Araújo; Nardin, Clezio Marcos de; Andrioli, Vania Fatima; Santos, Angela Machado; Picanco, Giorgio Arlan da Silva; Li, Hui; Zhengkuan, Liu; Wang, Chi; Schuch, Nelson Jorge
    Spread echoes from the E-region observed in ionograms obtained at high latitudes are generally classified as auroral sporadic-E (Esa) layers. These layers have also been detected in nighttime ionograms collected at some ionospheric stations in the South American Magnetic Anomaly (SAMA) region in Brazil during the recovery phases of geomagnetic storms. However, similar echoes have also been observed in the SAMA during geomagnetically quiet periods or daytime, which are not caused by energetic particle precipitation. Therefore, investigating the occurrence of these spread echoes over a longer period, rather than focusing solely on case studies, has become important. Thus, this study aims to analyze the occurrences of spread echoes from the E-region, referred to here for the first time as “Height-Spread Es (HSEs) layers.” The analysis is based on Digisonde data obtained at the Santa Maria station (29.7° S, 53.8° W, ∼22.000 nT) in Brazil over 1 year (2019/2020). The study initially presents examples of these traces on ionograms and then examines their occurrence rates over several time intervals (hours, months, seasons). Among other findings, the statistical analysis reveals that the occurrence rate of HSEs layers is 9.8% during the analyzed period. The HSEs layers appeared predominantly at night and under geomagnetically quiet conditions. Most HSEs layers lasted between 1 h and 3 h 30 min, with a peak incidence during November, December, and January. Finally, the study discusses the most likely mechanisms responsible for HSEs layer formation, considering the geomagnetic conditions and time of their detection on ionograms.

DSpace software copyright © 2002-2025 LYRASIS

  • Configurações de Cookies
  • Política de Privacidade
  • Termos de Uso
  • Enviar uma Sugestão
Desenvolvido por