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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.)

Multi-instrument study of longitudinal wave structures for plasma bubble seeding in the equatorial ionosphere

Texto completo
Autor(es):
Takahashi, H. [1] ; Essien, P. [1] ; Figueiredo, C. A. O. B. [1] ; Wrasse, C. M. [1] ; Barros, D. [1] ; Abdu, M. A. [1] ; Otsuka, Y. [2] ; Shiokawa, K. [2] ; Li, GuoZhu [3]
Número total de Autores: 9
Afiliação do(s) autor(es):
[1] Inst Nacl Pesquisas Espaciais, Sao Jose Dos Campos, SP - Brazil
[2] Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi - Japan
[3] Chinese Acad Sci, Inst Geol & Geophys, Beijing 100029 - Peoples R China
Número total de Afiliações: 3
Tipo de documento: Artigo Científico
Fonte: EARTH AND PLANETARY PHYSICS; v. 5, n. 5, SI, p. 368-377, SEP 2021.
Citações Web of Science: 1
Resumo

Large Scale Wave Structures (LSWS) in the equatorial ionospheric F-region were observed by measuring spatial and temporal variations within detrended total electron content (dTEC) data obtained by ground-based GNSS receivers over the South American continent. By using dTEC-maps, we have been able to produce, for the first-time, two-dimensional representations of LSWS. During the period from September to December, the LSWS frequently occurred starting a few hours prior to Equatorial Plasma Bubble (EPB) development. From 17 events of LSWS observed in 2014 and 2015, wave characteristics were obtained: the observed wavelengths, periods, and the phase speeds are respectively, similar to 900 km, similar to 41 min and similar to 399 m/s; the waves propagated from the northeast to southeast. In some cases the front of the oscillation was meridionally aligned, extending to more than 1600 km, the first time such large extension of the wavefront has been reported. From F-layer bottom height oscillation data, measured by ionosonde, LSWS exhibit two different vertical phase propagation modes, in-phase and downward phase. The former mode indicates the presence of a polarization electric field in the F-layer bottom side; the latter suggests propagation of atmospheric gravity waves. The presence of LSWS near the solar terminator, followed by the development of EPBs, suggests that the upwelling of the F-layer bottom height produces a condition favorable to the development of Rayleigh-Taylor instability. (AU)

Processo FAPESP: 18/09066-8 - Distúrbios ionosféricos propagantes observados sobre a cordilheira dos andes utilizando mapas/keogramas de conteúdo eletrônico total perturbado
Beneficiário:Cosme Alexandre Oliveira Barros Figueiredo
Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado