Gravity Wave Investigations over Comandante Ferraz Antarctic Station in 2017: General Characteristics, Wind Filtering and Case Study

Autor(es)

Giongo, Gabriel Augusto ^{[1, 2]} ; Bageston, Jose Valentin ^{[1, 2]} ; Oliveira Barros Figueiredo, Cosme Alexandre ^[3] ; Wrasse, Cristiano Max ^[3] ; Kam, Hosik ^{[4, 5]} ; Kim, Yong Ha ^[4] ; Schuch, Nelson Jorge ^[1]

Afiliação do(s) autor(es)

^[1] Natl Inst Space Res CRCRS COCRE INPE, Southern Reg Space Res Ctr, BR-97105900 Santa Maria, RS - Brazil

^[2] Univ Fed Santa Maria, Postgrad Program Meteorol PPGMet CCNE UFSM, BR-97105900 Santa Maria, RS - Brazil

^[3] Natl Inst Space Res DIDAE CGCEA INPE, Aeron Div, BR-12227010 Sao Jose Dos Campos - Brazil

^[4] Chungnam Natl Univ CNU, Dept Astron Space Sci & Geol, Daejeon 34134 - South Korea

^[5] Korea Polar Res Inst KOPRI, Div Polar Climate Sci, Incheon 21990 - South Korea

• Tipo de documento: Artigo Científico
• Fonte: ATMOSPHERE; v. 11, n. 8 AUG 2020.
• Citações Web of Science: 2

Resumo

This work presents the characteristics of gravity waves observed over Comandante Ferraz Antarctic Station (EACF: 62.1 degrees S, 58.4 degrees W). A total of 122 gravity waves were observed in 34 nights from March to October 2017, and their parameters were obtained by using the Fourier Transform spectral analysis. The majority of the observed waves presented horizontal wavelength ranging from 15 to 35 km, period from 5 to 20 min, and horizontal phase speed from 10 to 70 +/- 2 m center dot s(-1). The propagation direction showed an anisotropic condition, with the slower wave propagating mainly to the west, northwest and southeast directions, while the faster waves propagate to the east, southeast and south. Blocking diagrams for the period of April-July showed a good agreement between the wave propagation direction and the blocking positions, which are eastward oriented while the waves propagate mainly westward. A case study to investigate wave sources was conducted for the night of 20-21 July, wherein eight small-scale and one medium-scale gravity waves were identified. Reverse ray tracing model was used to investigate the gravity wave source, and the results showed that six among eight small-scale gravity waves were generated in the mesosphere. On the other hand, only two small-scale waves and the medium-scale gravity wave had likely tropospheric or stratospheric origin, however, they could not be associated with any reliable source. (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