Early Evolution of the Stratospheric Aerosol Plume Following the 2022 Hunga Tonga‐Hunga Ha'apai Eruption: Lidar Observations From Reunion (21°S, 55°E)

Author:

Baron A.123ORCID,Chazette P.4ORCID,Khaykin S.5ORCID,Payen G.6ORCID,Marquestaut N.6,Bègue N.1,Duflot V.1ORCID

Affiliation:

1. Laboratoire de l’Atmosphère et des Cyclones (LACy) UMR 8105 CNRS Université de la Réunion Météo‐France Saint‐Denis de La Réunion France

2. Now at Cooperative Institute for Research in Environmental Sciences CU Boulder Boulder CO USA

3. Now at NOAA Chemical Sciences Laboratory Boulder CO USA

4. Laboratoire des Sciences du Climat et de l'Environnement LSCE‐IPSL UMR 8212 Université Paris‐Saclay, CEA, CNRS, UVSQ Gif‐sur‐Yvette France

5. Laboratoire Atmosphère Milieux Observations Spatiales LATMOS‐IPSL UMR 8190 Sorbonne Université, UVSQ, CNRS Paris France

6. Observatoire des Sciences de l’Univers de La Réunion (OSU‐Réunion) UAR 3365 Université de la Réunion CNRS Météo‐France Saint‐Denis de La Réunion France

Abstract

AbstractThe exceptionally violent eruption of the Hunga Tonga‐Hunga Ha'apai volcano (HTHH) of 15 January 2022, in the South Pacific, was associated with a powerful blast that injected gases, steam and aerosol to unprecedentedly high altitudes. This article details unique observations of the young volcanic plume from ground‐based lidars at Reunion (21°S, 55°E). Two lidars, operating at wavelengths of 355 and 532 nm, recorded the plume overhead from 19 January until 28 January providing the vertical structure and the optical properties of the plume. A series of thick stratospheric plumes between 36 and 18 km altitude have been characterized along time, with aerosol optical depth as high as 0.84 at 532 nm and negative Angström exponents for the main layers down to −0.8 ± 0.8. The diversity of plumes properties is explained by the injection heights of the volcanic material as well as stratospheric dynamics and chemistry.

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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