Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/16251
Title: Global Response of Vertical Total Electron Content to Mother’s Day G5 Geomagnetic Storm of May 2024: Insights from IGS and GIM Observations
Authors: Brawar, Bhuvnesh
Datta, Abhirup
Keywords: GIM;global ionospheric map analysis;global VTEC anomalies;Mother’s Day Storm;temporal variation in VTEC
Issue Date: 2025
Publisher: Multidisciplinary Digital Publishing Institute (MDPI)
Citation: Pal, S. K., Sarkar, S., Nanda, K., Sanyal, A., Brawar, B., Datta, A., Potirakis, S. M., Maurya, A. K., Bhattacharya, A., Panchadhyayee, P., Ray, S., & Sasmal, S. (2025). Global Response of Vertical Total Electron Content to Mother’s Day G5 Geomagnetic Storm of May 2024: Insights from IGS and GIM Observations. Atmosphere. https://doi.org/10.3390/atmos16050529
Abstract: The G5 geomagnetic storm of May 2024 provided a significant opportunity to investigate global ionospheric disturbances using vertical total electron content (VTEC) data derived from 422 GNSS-IGS stations and GIM. This study presents a comprehensive spatio-temporal analysis of VTEC modulation before, during, and after the storm, focusing on hemispheric asymmetries and longitudinal variations. The primary objective of this study is to analyze the spatial and temporal modulation of VTEC under extreme geomagnetic conditions, assess the hemispheric asymmetry and longitudinal disruptions, and evaluate the influence of geomagnetic indices on storm-time ionospheric variability. The indices examined reveal intense geomagnetic activity, with the dst index plunging to −412 nT, the Kp index reaching 9, and significant fluctuations in the auroral electrojet indices (AE, AL, AU), all indicative of severe space weather conditions. The results highlight storm-induced hemispheric asymmetries, with positive storm effects (VTEC enhancement) in the Northern Hemisphere and negative storm effects (VTEC depletion) in the Southern Hemisphere. These anomalies are primarily attributed to penetration electric fields, neutral wind effects, and composition changes in the ionosphere. The storm’s peak impact on DoY 132 exhibited maximum disturbances at ±90° and ±180° longitudes, emphasizing the role of geomagnetic forces in plasma redistribution. Longitudinal gradients were strongly amplified, disrupting the usual equatorial ionization anomaly structure. Post-storm recovery on DoY 136 demonstrated a gradual return to equilibrium, although lingering effects persisted at mid- and high latitudes. These findings are crucial for understanding space weather-induced ionospheric perturbations, directly impacting GNSS-based navigation, communication systems, and space weather forecasting. © 2025 by the authors.
URI: https://dx.doi.org/10.3390/atmos16050529
https://dspace.iiti.ac.in:8080/jspui/handle/123456789/16251
ISSN: 2073-4433
Type of Material: Journal Article
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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