Analysis of Ionospheric TEC Variations Due to X, M & C Class Solar Flares during the Years 2003 to 2018 and Comparison with IRI Models
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Geophysics
Link
https://link.springer.com/content/pdf/10.1134/S0016793222080138.pdf
Reference28 articles.
1. Ansari, K., Park, K.D., and Panda, S.K., Empirical orthogonal function analysis and modeling of ionospheric TEC over South Korean region, Acta Astronaut., 2019, id 161.https://doi.org/10.1016/j.actaastro.2019.05.044
2. Bilitza, D., Altadill, D., Zhang, Y., and Christopher, M.T., The International Reference Ionosphere 2012: A model of international collaboration, J. Space Weather Space Clim., 2014, vol. 4, id A07. https://doi.org/10.1051/swsc/2014004
3. Recurrent ionospheric storms during solar minimum;A.V. Dmitriev,2015
4. Durga, R.K., Panda, S.K., and Dash, R.N., GPS satellite signals derived ionospheric TEC, and assessment of IRI-2016 and SPIM-2017 model predictions over Indian region, in Proceedings of the 2018 International Conference on Recent Innovations in Electrical, Electronics, and Communication Engineering (ICRIEECE), 2018, pp. 3237–3242. https://doi.org/10.1109/icrieece44171.2018.9008926.
5. Endalkachew, M., Mark, B.M., Baylie, D., and Melessew, N., The performance of IRI-2016 in the African sector of equatorial ionosphere for different geomagnetic conditions and time scales, J. Atmos. Sol.-Terr. Phys., 2019, vol. 186, pp. 116–138. https:// doi.org/.https://doi.org/10.1016/j.jastp.2019.02.006
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