Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 35, issue 4
Articles | Volume 35, issue 4
https://doi.org/10.5194/angeo-35-923-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
Special issue:
https://doi.org/10.5194/angeo-35-923-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
Articles | Volume 35, issue 4
Regular paper
 | 
09 Aug 2017
Regular paper |  | 09 Aug 2017

Similarity and differences in morphology and mechanisms of the foF2 and TEC disturbances during the geomagnetic storms on 26–30 September 2011

Maxim V. Klimenko, Vladimir V. Klimenko, Irina E. Zakharenkova, Konstantin G. Ratovsky, Nina A. Korenkova, Yury V. Yasyukevich, Anna A. Mylnikova, and Iurii V. Cherniak

Viewed

Total article views: 1,880 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,062 715 103 1,880 108 161
  • HTML: 1,062
  • PDF: 715
  • XML: 103
  • Total: 1,880
  • BibTeX: 108
  • EndNote: 161
Views and downloads (calculated since 09 Aug 2017)
Cumulative views and downloads (calculated since 09 Aug 2017)
Latest update: 22 Nov 2025
Download
Short summary
Using model–data analysis we emphasize a new result – formation of the positive daytime disturbances in foF2 and TEC at middle and low latitudes due to n(O)/n(N2) enhancement during the recovery storm phase. The spatial extent of this phenomenon depends on the longitudinal sector. The positive disturbances in the electron content at heights of 800–20 000 km at high latitudes can appear simultaneously with the negative disturbances in TEC and foF2 due to electron and neutral temperature heating.
Read more
Share
Special issue
The 14th International Symposium on Equatorial Aeronomy