Plasmas (LPP), CNRS, Sorbonne Université, Université Paris Saclay, Observatoire de Paris, Ecole polytechnique, Institut Polytechnique de Paris, Paris, France
Binod Adhikari
Department of Physics, Patan M. Campus, Tribhuvan University, Lalitpur, Nepal
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507
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PDF: 4,164
XML: 351
Total: 14,373
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Total article views: 660 (including HTML, PDF, and XML)
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529
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660
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HTML: 529
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Total: 660
Supplement: 49
BibTeX: 72
EndNote: 62
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Total article views: 13,713 (including HTML, PDF, and XML)
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9,329
4,093
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1,228
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HTML: 9,329
PDF: 4,093
XML: 291
Total: 13,713
Supplement: 1,228
BibTeX: 318
EndNote: 445
Views and downloads (calculated since 30 Jan 2025)
Cumulative views and downloads
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Viewed (geographical distribution)
Total article views: 14,373 (including HTML, PDF, and XML)
Thereof 14,187 with geography defined
and 186 with unknown origin.
Total article views: 660 (including HTML, PDF, and XML)
Thereof 594 with geography defined
and 66 with unknown origin.
Total article views: 13,713 (including HTML, PDF, and XML)
Thereof 13,593 with geography defined
and 120 with unknown origin.
Comprehensive analysis of geomagnetic storms from 23–25 March, 23–25 April, 4–6 November 2023, and 10–13 May 2024, reveals that solar wind parameters, geomagnetic activity, Joule heating, and Prompt Penetration Electric Fields significantly influence ionospheric Total Electron Content variations, Equatorial Ionization Anomaly crest formations, and post-sunset plasma irregularities. The storms highlighted the importance of inter-hemispheric asymmetries in Joule Heating, which affected the distribution and magnitude of ionospheric disturbances.
Comprehensive analysis of geomagnetic storms from 23–25 March, 23–25 April, 4–6 November 2023,...