Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/16251
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dc.contributor.authorBrawar, Bhuvneshen_US
dc.contributor.authorDatta, Abhirupen_US
dc.date.accessioned2025-06-16T05:48:07Z-
dc.date.available2025-06-16T05:48:07Z-
dc.date.issued2025-
dc.identifier.citationPal, 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/atmos16050529en_US
dc.identifier.issn2073-4433-
dc.identifier.otherEID(2-s2.0-105006670480)-
dc.identifier.urihttps://dx.doi.org/10.3390/atmos16050529-
dc.identifier.urihttps://dspace.iiti.ac.in:8080/jspui/handle/123456789/16251-
dc.description.abstractThe 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.en_US
dc.language.isoenen_US
dc.publisherMultidisciplinary Digital Publishing Institute (MDPI)en_US
dc.sourceAtmosphereen_US
dc.subjectGIMen_US
dc.subjectglobal ionospheric map analysisen_US
dc.subjectglobal VTEC anomaliesen_US
dc.subjectMother’s Day Stormen_US
dc.subjecttemporal variation in VTECen_US
dc.titleGlobal Response of Vertical Total Electron Content to Mother’s Day G5 Geomagnetic Storm of May 2024: Insights from IGS and GIM Observationsen_US
dc.typeJournal Articleen_US
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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