Articles | Volume 37, issue 6
https://doi.org/10.5194/angeo-37-1141-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Special issue:
https://doi.org/10.5194/angeo-37-1141-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Regular paper
| 
10 Dec 2019
Regular paper |
| 10 Dec 2019
| 10 Dec 2019
Long-term trends in the ionospheric response to solar extreme-ultraviolet variations
Rajesh Vaishnav
CORRESPONDING AUTHOR
Leipzig Institute for Meteorology, Universität Leipzig, Stephanstr. 3, 04103 Leipzig, Germany
Christoph Jacobi
Leipzig Institute for Meteorology, Universität Leipzig, Stephanstr. 3, 04103 Leipzig, Germany
Jens Berdermann
German Aerospace Center, Kalkhorstweg 53, 17235 Neustrelitz, Germany
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- The Height‐Dependent Delayed Ionospheric Response to Solar EUV E. Schmölter et al. 10.1029/2021JA030118
- Ionospheric anomalies associated with the <i>M</i><sub>w</sub> 7.3 Iran–Iraq border earthquake and a moderate magnetic storm E. Şentürk et al. 10.5194/angeo-38-1031-2020
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- Ionospheric anomalies detection using autoregressive integrated moving average (ARIMA) model as an earthquake precursor M. Saqib et al. 10.1007/s11600-021-00616-3
- Persistent perturbations of ionosphere at diminution of solar and geomagnetic activity during 21–24 solar cycles T. Gulyaeva et al. 10.1016/j.jastp.2021.105706
- Selecting the best solar EUV proxy for long-term timescale applications B. Zossi et al. 10.1016/j.asr.2024.07.023
- Enhanced Forecasting of Global Ionospheric Vertical Total Electron Content Maps Using Deep Learning Methods Y. Lin et al. 10.3390/atmos15111319
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- Ionospheric anomalies related to the Mw 6.5 Samar, Philippines earthquake E. Eroglu 10.1007/s11600-022-00980-8
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- An EOF-Based Global Plasmaspheric Electron Content Model and Its Potential Role in Vertical-Slant TEC Conversion F. Long et al. 10.3390/rs16111857
- Analysis of ionospheric TEC response to solar and geomagnetic activities at different solar activity stages J. Feng et al. 10.1016/j.asr.2022.10.032
- Intensity of 27-day variations in solar emission and ionospheric electron content A. Setov et al. 10.1016/j.asr.2024.10.054
- Decomposing solar and geomagnetic activity and seasonal dependencies to examine the relationship between GPS loss of lock and ionospheric turbulence G. Lovati et al. 10.1038/s41598-023-34727-2
- Ionospheric Response to Solar EUV Radiation Variations Using GOLD Observations and the CTIPe Model R. Vaishnav et al. 10.1029/2022JA030887
- Persistent high-latitude ionospheric response to solar wind forcing C. Borries et al. 10.1051/swsc/2024029
- Role of eddy diffusion in the delayed ionospheric response to solar flux changes R. Vaishnav et al. 10.5194/angeo-39-641-2021
- Solar Activity Driven 27‐Day Signatures in Ionospheric Electron and Molecular Oxygen Densities E. Schmölter & C. von Savigny 10.1029/2022JA030671
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- Swarm Langmuir probes' data quality validation and future improvements F. Catapano et al. 10.5194/gi-11-149-2022
- The best solar activity proxy for long-term ionospheric investigations J. Laštovička 10.1016/j.asr.2021.06.032
- What is the optimum solar proxy for long-term ionospheric investigations? J. Laštovička 10.1016/j.asr.2020.07.025
- Low latitude monthly total electron content composite correlations D. Allen et al. 10.1051/swsc/2023005
- Delayed ionospheric response to solar extreme ultraviolet radiation variations: A modeling approach R. Vaishnav et al. 10.1016/j.asr.2021.12.041
- Ionospheric response to solar extreme ultraviolet radiation variations: comparison based on CTIPe model simulations and satellite measurements R. Vaishnav et al. 10.5194/angeo-39-341-2021
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- Responding trends of ionosphericF2-layer to weaker geomagnetic activities Y. Chen et al. 10.1051/swsc/2022005
- Evaluation for effects of variable Martian upper atmosphere on ionospheric peak electron density based on the MGS RO observation Y. Chen et al. 10.1016/j.icarus.2022.115364
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Latest update: 20 Nov 2024
Short summary
We investigate the ionospheric response to the temporal and spatial dynamics of the solar activity using total electron content (TEC) maps and multiple solar proxies. The maximum correlation at a 16–32-d timescale is observed between the He-II, Mg-II, and F30 with respect to global mean TEC, with an effective time delay of about 1 d. The most suitable proxy to represent the solar activity at the timescales of 16–32 d and 32–64 d is He-II.
We investigate the ionospheric response to the temporal and spatial dynamics of the solar...
Special issue