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.
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.
the Creative Commons Attribution 3.0 License.
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
CORRESPONDING AUTHOR
West Department of Pushkov IZMIRAN, RAS, Kaliningrad, Russia
Immanuel Kant Baltic Federal University, Kaliningrad, Russia
Vladimir V. Klimenko
West Department of Pushkov IZMIRAN, RAS, Kaliningrad, Russia
Irina E. Zakharenkova
West Department of Pushkov IZMIRAN, RAS, Kaliningrad, Russia
Konstantin G. Ratovsky
Institute of Solar-Terrestrial Physics, SB RAS, Irkutsk, Russia
Nina A. Korenkova
West Department of Pushkov IZMIRAN, RAS, Kaliningrad, Russia
Yury V. Yasyukevich
Institute of Solar-Terrestrial Physics, SB RAS, Irkutsk, Russia
Anna A. Mylnikova
Institute of Solar-Terrestrial Physics, SB RAS, Irkutsk, Russia
Iurii V. Cherniak
University of Warmia and Mazury, Olsztyn, Poland
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Latest update: 20 Nov 2024
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.
Using model–data analysis we emphasize a new result – formation of the positive daytime...
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