Articles | Volume 35, issue 3
https://doi.org/10.5194/angeo-35-763-2017
https://doi.org/10.5194/angeo-35-763-2017
Regular paper
 | 
22 Jun 2017
Regular paper |  | 22 Jun 2017

Features of 3–7-day planetary-wave-type oscillations in F-layer vertical drift and equatorial spread F observed over two low-latitude stations in China

Zhengping Zhu, Weihua Luo, Jiaping Lan, and Shanshan Chang

Viewed

Total article views: 1,480 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
862 547 71 1,480 60 70
  • HTML: 862
  • PDF: 547
  • XML: 71
  • Total: 1,480
  • BibTeX: 60
  • EndNote: 70
Views and downloads (calculated since 22 Jun 2017)
Cumulative views and downloads (calculated since 22 Jun 2017)

Cited

Latest update: 14 Dec 2024
Download
Short summary
Features of planetary waves in Chinese low-latitude regions are investigated. Planetary waves are observed in both MLT winds and ionospheric vertical drifts. ESF occurrence is with the uplift of the F layer caused by PRE, and a delay of about 6 days is observed for planetary waves propagating from the lower atmosphere to the ionosphere. This investigation contributes to the understanding of atmosphere–ionosphere coupling processes and the effects of planetary waves on ESF.