An Analysis of Ionospheric Conditions during Intense Geomagnetic Storms (Dst ≤ −100 nt) in the Period 2011–2018
Author:
Affiliation:
1. Faculty of Earth and Space Sciences, Autonomous University of Sinaloa, Culiacán 80040, Mexico
2. Department of Applied Geophysics, Center for Scientific Research and Higher Education of Ensenada, Tijuana 22860, Mexico
Publisher
MDPI
Link
https://www.mdpi.com/2673-4931/27/1/18/pdf
Reference10 articles.
1. López-Urias, C., Vazquez-Becerra, G.E., Nayak, K., and López-Montes, R. (2023). Analysis of Ionospheric Disturbances during X-Class Solar Flares (2021–2022) Using GNSS Data and Wavelet Analysis. Remote Sens., 15.
2. Validation of computed extreme ultraviolet emission spectra during solar flares;Nishimoto;Earth Planets Space,2021
3. The 6 September 2017 X-class solar flares and their impacts on the ionosphere, GNSS, and HF radio wave propagation;Yasyukevich;Space Weather.,2018
4. Pelton, J., and Allahdadi, F. (2015). Handbook of Cosmic Hazards and Planetary Defense, Springer.
5. Singh, A.K., Bhargawa, A., Siingh, D., and Singh, R.P. (2021). Physics of Space Weather Phenomena: A Review. Geosciences, 11.
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