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Aerosol characterization of the stratospheric plume from the volcanic eruption at Hunga Tonga January 15th 2022
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  • Corinna Kloss,
  • Pasquale Sellitto,
  • jean-baptiste renard,
  • Alexandre Baron,
  • Nelson BEGUE,
  • Bernard Legras,
  • Gwenael Berthet,
  • Emmanuel Briaud,
  • Elisa Carboni,
  • Clair Duchamp,
  • Valentin Duflot,
  • Patrick Jacquet,
  • Nicolas Marquestaut,
  • Jean-Marc Metzger,
  • Guillaume Payen,
  • Marion Ranaivombola,
  • Tjarda Roberts,
  • Richard Siddans,
  • Fabrice Jegou
Corinna Kloss
Laboratoire de Physique et Chimie de l'Environment et de l'Espace (LPC2E), CNRS

Corresponding Author:[email protected]

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Pasquale Sellitto
Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA-IPSL)
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jean-baptiste renard
CNRS
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Alexandre Baron
University of La Réunion
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Nelson BEGUE
Laboratoire de l'atmosphere et des Cyclones-Universite de la Reunion
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Bernard Legras
Ecole Normale Superieure
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Gwenael Berthet
French National Centre for Scientific Research (CNRS)
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Emmanuel Briaud
French National Centre for Scientific Research (CNRS)
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Elisa Carboni
University of Oxford
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Clair Duchamp
Ecole Normale Superieure
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Valentin Duflot
LACy UMR8105/OSUR
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Patrick Jacquet
French National Centre for Scientific Research (CNRS)
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Nicolas Marquestaut
Observatoire des Sciences de l'Univers de La Réunion
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Jean-Marc Metzger
OSUR
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Guillaume Payen
OSUR
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Marion Ranaivombola
Laboratoire de l'Atmosphere et des Cyclones-Université de la Reunion
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Tjarda Roberts
CNRS
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Richard Siddans
Rutherford Appleton Laboratory
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Fabrice Jegou
LPC2E / French National Centre for Scientific Research (CNRS)
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Abstract

Following the Hunga Tonga eruption (20.6°S, 175.4°W, mid-January 2022), we present a balloon-borne characterization of the stratospheric aerosol plume one week after its injection (on 23 and 26/01/2022, La Réunion island at 21.1°S, 55.3°E). Satellite observations show that flight #1 took place during the overpass of a denser plume of sulfate aerosols (SA) compared to a more diluted plume during flight #2. Observations show that the sampled plumes (at around 22, 25 and 19 km altitude, respectively) consist exclusively of very small particles (with radius < 1 µm). Particles with radii between 0.5 and 1.0 µm show optically transparent features pointing to predominant SA. Particles with radii below 0.5 µm are partly absorbing, which could point to small sulfate coated ash particles, a feature not identified with space-borne observations. This shows that in situ observations are necessary to fully characterize the microphysical properties of the plumes tracked by space-borne instruments.