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Atmospheric gravity waves observed in the nightglow following the 21 August 2017 total solar eclipse}
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  • Igo Paulino,
  • Cosme A. O. B. Figueiredo,
  • Fabiano Rodrigues,
  • Ricardo A. Buriti,
  • Cristiano M. Wrasse,
  • Ana Roberta Paulino,
  • Diego Barros,
  • Hisao Takahashi,
  • Inez S. Batista,
  • A. F. Medeiros,
  • Paulo Prado Prado Batista,
  • Mangalathayil Ali Abdu,
  • Eurico Rodrigues de Paula,
  • Clezio Marcos Denardini,
  • Lourivaldo M. Lima,
  • Ricardo Y.C. Cueva,
  • Jonathan J. Makela
Igo Paulino
Universidade Federal de Campina Grande

Corresponding Author:[email protected]

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Cosme A. O. B. Figueiredo
Instituto Nacional de Pesquisas Espaciais
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Fabiano Rodrigues
UT Dallas
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Ricardo A. Buriti
Universidade Federal de Campina Grande
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Cristiano M. Wrasse
Instituto Nacional de Pesquisas Espaciais
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Ana Roberta Paulino
Universidade Federal de Campina Grande
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Diego Barros
Instituto Nacional de Pesquisas Espaciais
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Hisao Takahashi
Instituto Nacional de Pesquisas Espaciais
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Inez S. Batista
National Institute for Space Research
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A. F. Medeiros
Universidade Federal de Campina Grande
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Paulo Prado Prado Batista
Instituto Nacional de Pesquisas Espacia
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Mangalathayil Ali Abdu
Instituto Nacional de Pesquisas Espaciais
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Eurico Rodrigues de Paula
Instituto Nacional de Pesquisas Espaciais
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Clezio Marcos Denardini
National Institute for Space Research
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Lourivaldo M. Lima
Universidade Estadual de Paraiba
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Ricardo Y.C. Cueva
State University of Maranhao
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Jonathan J. Makela
University of Illinois at Urbana Champaign
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Abstract

Nighttime airglow images observed at the low-latitude site of São João do Cariri (7.4S, 36.5W) showed the presence of a medium-scale atmospheric gravity wave (AGW) associated with the 21 August 2017 total solar eclipse. The AGW had a horizontal wavelength of ~1,618 km, observed period of ~152 min and propagation direction of ~200 clockwise from the north. The spectral characteristics of this wave are in good agreement with theoretical predictions for waves generated by eclipses. Additionally, the wave was reverse ray-traced and the results show its path crossing the Moon’s shadow of the total solar eclipse in the tropical North Atlantic ocean at stratospheric altitudes. Investigation about potential driving sources for this wave indicate that the total solar eclipse as the most likely candidate. The optical measurements were part of an observational campaign carried out to detect the impact of the August 21 eclipse in the atmosphere at low latitudes.
16 Sep 2020Published in Geophysical Research Letters volume 47 issue 17. 10.1029/2020GL088924