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Extreme poleward expanding super plasma bubbles triggered by Tonga volcano eruption during the recovery phase of geomagnetic storm
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  • P. K. Rajesh,
  • Charles C. H. Lin,
  • Jia-Ting Lin,
  • Chi-Yen Lin,
  • Jann-Yenq Liu,
  • Tomoko Matsuo,
  • Cheng-Yung Huang,
  • Min-Yang Chou,
  • Jia Yue,
  • Michi Nishioka,
  • Hidekatsu Jin,
  • Jong-Min Choi,
  • Shih-Ping Chen,
  • Marty Chou,
  • Ho-Fang Tsai
P. K. Rajesh
National Cheng Kung University
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Charles C. H. Lin
National Cheng Kung University

Corresponding Author:[email protected]

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Jia-Ting Lin
National Cheng Kung University
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Chi-Yen Lin
National Central University
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Jann-Yenq Liu
National Central University
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Tomoko Matsuo
Ann and H.J. Smead Department of Aerospace Engineering Sciences, University of Colorado Boulder
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Cheng-Yung Huang
National Central University
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Min-Yang Chou
Goddard Space Flight Center
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Jia Yue
Goddard Space Flight Center
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Michi Nishioka
National Institute of Information and Communications Technology
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Hidekatsu Jin
National Institute of Information and Communications Technology
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Jong-Min Choi
National Cheng Kung University
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Shih-Ping Chen
National Cheng Kung University
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Marty Chou
National Cheng Kung University
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Ho-Fang Tsai
National Central University
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Abstract

The Tonga volcano eruption of 15 January 2022 unleashed a variety of atmospheric perturbations, coinciding with the recovery phase of a geomagnetic storm. The ensuing thermospheric variations created rare display of extreme poleward-expanding conjugate plasma bubbles seen in the rate of total electron content index (ROTI) over 100-150°E. This is associated with fluctuations in FORMOSAT-7/COSMIC-2 (F7/C2) ion-density measurements and spread-F signatures in ionograms, reaching ~40°N geographic latitude. This was preceded by an unusually strong pre-reversal enhancement (PRE) in the global ionospheric specification (GIS) electron density profiles derived from F7/C2 observations. The GIS further revealed a decrease of equatorial ionization anomaly (EIA) crest density due to the storm impact. A sharp decrease of E-region conductivity by volcano-induced waves, combined with enhanced F-region wind over EIA with less ion-drag apparently intensified the PRE. The strong PRE and seed perturbations from the volcano-induced waves likely further triggered super plasma bubble activity.