Articles | Volume 36, issue 2
https://doi.org/10.5194/angeo-36-459-2018
https://doi.org/10.5194/angeo-36-459-2018
Regular paper
 | 
21 Mar 2018
Regular paper |  | 21 Mar 2018

Wavenumber-4 structures observed in the low-latitude ionosphere during low and high solar activity periods using FORMOSAT/COSMIC observations

Amelia Naomi Onohara, Inez Staciarini Batista, and Paulo Prado Batista

Viewed

Total article views: 1,996 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,249 655 92 1,996 84 79
  • HTML: 1,249
  • PDF: 655
  • XML: 92
  • Total: 1,996
  • BibTeX: 84
  • EndNote: 79
Views and downloads (calculated since 21 Mar 2018)
Cumulative views and downloads (calculated since 21 Mar 2018)

Cited

Latest update: 12 Dec 2024
Download
Short summary
Global coverage measurements made by satellites have provided observational studies which have shown the presence of four peaks in global longitudinal structures from global local time observations of equatorial ionization anomalies. The structures seen in the ionosphere are related to the diurnal non-migrating wave that comes from the troposphere and can be noticed in periods of low and high solar activity in the low-latitude ionosphere regions, mainly at altitudes from ~ 250 km up to ~ 800 km.