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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Ionospheric Response to Disturbed Winds During the 29 October 2003 Geomagnetic Storm in the Brazilian Sector

Texto completo
Autor(es):
Bravo, M. A. [1, 2] ; Batista, I. S. [1] ; Souza, J. R. [1] ; Foppiano, A. J. [2]
Número total de Autores: 4
Afiliação do(s) autor(es):
[1] INPE, Sao Jose Dos Campos - Brazil
[2] Univ Concepcion, UdeC, Dept Geofis, Concepcion - Chile
Número total de Afiliações: 2
Tipo de documento: Artigo Científico
Fonte: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS; v. 124, n. 11 NOV 2019.
Citações Web of Science: 0
Resumo

Modeling the ionosphere during disturbed periods is one of the most challenging tasks due to the complexity of the phenomena that affect the electric fields and the whole thermosphere environment. It is well known that both, prompt penetration electric fields and large amounts of energy deposited in the polar region during disturbed periods, produce significant disturbances in the global electron density distribution, in particular, in the equatorial ionization anomaly development. Besides, the disturbance dynamo, traveling atmospheric disturbances, and traveling ionospheric disturbances also affect the equatorial ionization anomaly density distribution. In this work we use the Sheffield University Plasmasphere-Ionosphere Model at Instituto Nacional de Pesquisas Espaciais, to simulate the drastic effects that were observed at the low-latitude ionosphere in the Brazilian region during a very intense magnetic storm event, the so-called 2003 Halloween storms. In the absence of measured vertical drift during the storm, a new vertical drift deduced from the interplanetary electric field combined with the time variation of the F region virtual height is used as input. The simulation results showed that, in the case of the disturbed thermospheric wind, the ionospheric observations are better explained when a novel traveling wave-like disturbance propagating from north to south, at a velocity equal to 300 m/s, is considered. (AU)

Processo FAPESP: 17/50115-0 - INCT 2014: tecnologia GNSS no suporte à navegação aérea
Beneficiário:Joao Francisco Galera Monico
Modalidade de apoio: Auxílio à Pesquisa - Pesquisa em Políticas Públicas