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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4,096
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13,770
1,227
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446
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PDF: 4,096
XML: 293
Total: 13,770
Supplement: 1,227
BibTeX: 322
EndNote: 446
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Cumulative views and downloads
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Total article views: 153 (including HTML, PDF, and XML)
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119
26
8
153
18
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Total: 153
Supplement: 18
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EndNote: 7
Views and downloads (calculated since 23 Jun 2026)
Cumulative views and downloads
(calculated since 23 Jun 2026)
Total article views: 13,617 (including HTML, PDF, and XML)
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9,262
4,070
285
13,617
1,209
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439
HTML: 9,262
PDF: 4,070
XML: 285
Total: 13,617
Supplement: 1,209
BibTeX: 314
EndNote: 439
Views and downloads (calculated since 30 Jan 2025)
Cumulative views and downloads
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Viewed (geographical distribution)
Total article views: 13,770 (including HTML, PDF, and XML)
Thereof 13,643 with geography defined
and 127 with unknown origin.
Total article views: 153 (including HTML, PDF, and XML)
Thereof 121 with geography defined
and 32 with unknown origin.
Total article views: 13,617 (including HTML, PDF, and XML)
Thereof 13,522 with geography defined
and 95 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,...