Geomagnetic Storms and Their Consequences: Advances in Prediction Models

A special issue of Atmosphere (ISSN 2073-4433). This special issue belongs to the section "Upper Atmosphere".

Deadline for manuscript submissions: 30 June 2026 | Viewed by 405

Special Issue Editor


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Guest Editor
National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing, China
Interests: space weather; solar energetic particles; geomagnetic storm
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Special Issue Information

Dear Colleagues,

We are pleased to announce a Special Issue dedicated to “Geomagnetic Storms and Their Consequences: Advances in Prediction Models”, inviting high-quality research articles, reviews, and case studies that focus on the dynamic interactions between solar wind, the magnetosphere, the ionosphere, and the upper atmosphere, especially geomagnetic storms and their consequences.

Geomagnetic storms, which are triggered by solar wind perturbations, can profoundly impact the ionosphere and thermosphere, disrupting satellite operations, radio communications, and navigation systems. This Special Issue seeks to advance our understanding of storm time phenomena, including ionospheric irregularities, thermospheric heating, and the coupling mechanisms between magnetospheric, ionospheric, and atmospheric layers. Contributions leveraging ground-based observations, satellite data, numerical modeling, and machine learning approaches are particularly encouraged.

Topics of interest include, but are not limited to, the following:

  • Storm-induced ionospheric plasma irregularities and scintillations.
  • Thermospheric composition and density changes during storms.
  • Magnetosphere–ionosphere–thermosphere coupling processes.
  • Impacts on GNSS, radar, and HF communication systems.
  • Long-term trends in space weather effects on the upper atmosphere.

Dr. Mingxian Zhao
Guest Editor

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Keywords

  • geomagnetic storm
  • space weather
  • upper atmosphere
  • thermosphere
  • ionosphere
  • magnetosphere
  • solar–terrestrial relations

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Published Papers (1 paper)

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Research

32 pages, 3525 KB  
Article
Discovery of Regular Daily Ionospheric Scintillation
by Janis Balodis, Madara Normand and Ingus Mitrofanovs
Atmosphere 2025, 16(12), 1330; https://doi.org/10.3390/atmos16121330 - 25 Nov 2025
Viewed by 216
Abstract
The aim of this study was to find out whether, just like in March 2015, daily regular GPS positioning disturbances caused by ionospheric scintillations occurred in other months of the solar activity cycle 24. The GPS positioning 90-s kinematic solutions of selected 46 [...] Read more.
The aim of this study was to find out whether, just like in March 2015, daily regular GPS positioning disturbances caused by ionospheric scintillations occurred in other months of the solar activity cycle 24. The GPS positioning 90-s kinematic solutions of selected 46 months covering 11 years were used to search for regular daily scintillation events. The hypothesis on predictable regular daily ionospheric scintillation was tested. Scintillation waves were discovered as a result of space weather impact with the sidereal day regularity. It leads to the conclusion that the radiation originates from the interplanetary medium. The enhancement of radiation waves by solar activity is similar to Pc1 waves. The regular daily ionospheric scintillation waves are recorded at any time of the day. In the years with low solar activity in 2010 and 2012, regular scintillation waves were not found. It cannot be claimed that the comparison of daily regular ionospheric scintillation cases over time with the mentioned Pc1 wave cases indicates any interrelation. Full article
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