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Pronounced Suppression and X-Pattern Merging of Equatorial Ionization Anomalies After the 2022 Tonga Volcano Eruption.
Aa, Ercha; Zhang, Shun-Rong; Wang, Wenbin; Erickson, Philip J; Qian, Liying; Eastes, Richard; Harding, Brian J; Immel, Thomas J; Karan, Deepak K; Daniell, Robert E; Coster, Anthea J; Goncharenko, Larisa P; Vierinen, Juha; Cai, Xuguang; Spicher, Andres.
Affiliation
  • Aa E; Haystack Observatory Massachusetts Institute of Technology Westford MA USA.
  • Zhang SR; Haystack Observatory Massachusetts Institute of Technology Westford MA USA.
  • Wang W; High Altitude Observatory National Center for Atmospheric Research Boulder CO USA.
  • Erickson PJ; Haystack Observatory Massachusetts Institute of Technology Westford MA USA.
  • Qian L; High Altitude Observatory National Center for Atmospheric Research Boulder CO USA.
  • Eastes R; Laboratory for Atmospheric and Space Physics University of Colorado Boulder CO USA.
  • Harding BJ; Space Sciences Laboratory University of California Berkeley CA USA.
  • Immel TJ; Space Sciences Laboratory University of California Berkeley CA USA.
  • Karan DK; Laboratory for Atmospheric and Space Physics University of Colorado Boulder CO USA.
  • Daniell RE; Ionospheric Physics Stoughton MA USA.
  • Coster AJ; Haystack Observatory Massachusetts Institute of Technology Westford MA USA.
  • Goncharenko LP; Haystack Observatory Massachusetts Institute of Technology Westford MA USA.
  • Vierinen J; Department of Physics and Technology The Arctic University of Norway Tromsø Norway.
  • Cai X; Laboratory for Atmospheric and Space Physics University of Colorado Boulder CO USA.
  • Spicher A; Department of Physics and Technology The Arctic University of Norway Tromsø Norway.
J Geophys Res Space Phys ; 127(6): e2022JA030527, 2022 Jun.
Article in En | MEDLINE | ID: mdl-35864906
Following the 2022 Tonga Volcano eruption, dramatic suppression and deformation of the equatorial ionization anomaly (EIA) crests occurred in the American sector ∼14,000 km away from the epicenter. The EIA crests variations and associated ionosphere-thermosphere disturbances were investigated using Global Navigation Satellite System total electron content data, Global-scale Observations of the Limb and Disk ultraviolet images, Ionospheric Connection Explorer wind data, and ionosonde observations. The main results are as follows: (a) Following the eastward passage of expected eruption-induced atmospheric disturbances, daytime EIA crests, especially the southern one, showed severe suppression of more than 10 TEC Unit and collapsed equatorward over 10° latitudes, forming a single band of enhanced density near the geomagnetic equator around 14-17 UT, (b) Evening EIA crests experienced a drastic deformation around 22 UT, forming a unique X-pattern in a limited longitudinal area between 20 and 40°W. (c) Thermospheric horizontal winds, especially the zonal winds, showed long-lasting quasi-periodic fluctuations between ±200 m/s for 7-8 hr after the passage of volcano-induced Lamb waves. The EIA suppression and X-pattern merging was consistent with a westward equatorial zonal dynamo electric field induced by the strong zonal wind oscillation with a westward reversal.
Key words

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: J Geophys Res Space Phys Year: 2022 Document type: Article Country of publication: United States

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: J Geophys Res Space Phys Year: 2022 Document type: Article Country of publication: United States