Periodic waves in the lower thermosphere observed by OI630 nm airglow images

Autor(es):Mostrar menos -

Paulino, I. ^[1] ; Medeiros, A. F. ^[1] ; Vadas, S. L. ^[2] ; Wrasse, C. M. ^[3] ; Takahashi, H. ^[3] ; Buriti, R. A. ^[1] ; Leite, D. ^[1] ; Filgueira, S. ^[1] ; Bageston, J. V. ^[3] ; Sobral, J. H. A. ^[3] ; Gobbi, D. ^[3]

Afiliação do(s) autor(es)

^[1] Univ Fed Campina Grande, Unidade Acad Fis, Campina Grande, PB - Brazil

^[2] Northwest Res Associates, Colorado Res Associates, Boulder, CO 80301 - USA

^[3] Inst Nacl Pesquisas Espaciais, Div Aeron, BR-12201 Sao Jose Dos Campos - Brazil

• Tipo de documento: Artigo Científico
• Fonte: Annales Geophysicae; v. 34, n. 2, p. 293-301, 2016.
• Citações Web of Science: 14

Resumo

Periodic wave structures in the thermosphere have been observed at Sao Joao do Cariri (geographic coordinates: 36.5 degrees W, 7.4 degrees S; geomagnetic coordinates based on IGRF model to 2015: 35.8 degrees E, 0.48 degrees N) from September 2000 to November 2010 using OI630.0 nm airglow images. During this period, which corresponds to almost one solar cycle, characteristics of 98 waves were studied. Similarities between the characteristics of these events and observations at other places around the world were noted, primarily the spectral parameters. The observed periods were mostly found between 10 and 35 min; horizontal wavelengths ranged from 100 to 200 km, and phase speed from 30 to 180ms(-1). These parameters indicated that some of the waves, presented here, are slightly faster than those observed previously at low and middle latitudes (Indonesia, Carib and Japan), indicating that the characteristics of these waves may change at different places. Most of observed waves have appeared during magnetically quiet nights, and the occurrence of those waves followed the solar activity. Another important characteristic is the quasi-monochromatic periodicity that distinguish them from the single-front medium-scale traveling ionospheric disturbances (MSTIDs) that have been observed previously over the Brazilian region. Moreover, most of the observed waves did not present a phase front parallel to the northeast-southwest direction, which is predicted by the Perkins instability process. It strongly suggests that most of these waves must have had different generation mechanisms from the Perkins instability, which have been pointed out as being a very important mechanism for the generation of MSTIDs in the lower thermosphere. (AU)

• Processo FAPESP: 11/20120-5 - Modelo regional de propagação de ondas de gravidade atmosféricas
• Beneficiário: Igo Paulino da Silva
• Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado