Aerosol Characterization of the Stratospheric Plume From the Volcanic Eruption at Hunga Tonga 15 January 2022

被引:19
|
作者
Kloss, Corinna [1 ]
Sellitto, Pasquale [2 ,3 ,4 ]
Renard, Jean-Baptiste [1 ]
Baron, Alexandre [5 ]
Begue, Nelson [5 ]
Legras, Bernard [6 ]
Berthet, Gwenael [1 ]
Briaud, Emmanuel [1 ]
Carboni, Elisa [7 ]
Duchamp, Clair [6 ]
Duflot, Valentin [5 ]
Jacquet, Patrick [1 ]
Marquestaut, Nicolas [8 ]
Metzger, Jean-Marc [8 ]
Payen, Guillaume [8 ]
Ranaivombola, Marion [5 ]
Roberts, Tjarda [1 ]
Siddans, Richard [7 ]
Jegou, Fabrice [1 ]
机构
[1] Univ Orleans, Lab Phys & Chim Environm & Espace LPC2E, CNRS, UMR 7328, Orleans, France
[2] Univ Paris Est Creteil, Creteil, France
[3] Univ Paris Cite, Lab Interuniv Syst Atmospher LISA, Inst Pierre Simon Laplace IPSL, CNRS, Creteil, France
[4] Osservatorio Etneo, Ist Nazl Geofis & Vulcanol, Catania, Italy
[5] Univ Reunion, Lab Atmosphere & Cyclones LACy, CNRS, UMR 8105,Meteo France, St Denis, France
[6] Sorbonne Univ, Lab Meteorol Dynam, UMR CNRS, ENS PSL,Ecole Polytech, Paris, France
[7] UK Res & Innovat Sci & Technol Facil Council, Rutherford Appleton Lab, Chilton, England
[8] Univ Reunion, Observ Sci Univers Reunion OSUR, CNRS, Meteo France,UAR 3365, St Denis, France
关键词
Hunga Tonga; in situ observations; stratosphere; aerosol plume; aerosol size distribution; aerosol typology; SIZE DISTRIBUTION; SULFATE AEROSOLS; IN-SITU; LIDAR; PROFILES;
D O I
10.1029/2022GL099394
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Following the Hunga Tonga eruption (20.6 degrees S, 175.4 degrees W, mid-January 2022), we present a balloon-borne characterization of the stratospheric aerosol plume one week after its injection (on 23 and 26 January 2022, La Reunion island at 21.1 degrees S, 55.3 degrees E). Satellite observations show that flight (a) took place during the overpass of a denser plume of sulfate aerosols (SA) compared to a more diluted plume during flight. (b) Observations show that the sampled plumes (at around 22, 25 and 19 km altitude, respectively) consist exclusively of very small particles (with radius <1 mu m). Particles with radii between 0.5 and 1.0 mu m show optically transparent features pointing to predominant SA. Particles with radii below 0.5 mu m 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.
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页数:9
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