Reconstruction of flux and altitude of volcanic SO2 emissions from IASI satellite observations: implications for volcanological and atmospherical studies.

Abstract : Volcanic SO2 degassing is a crucial indicator of the sub-surface volcanic activity, which is widely used today for volcano monitoring and hazard assessment purposes. Volcanic SO2 is also important regarding atmospherical studies. More easily detectable from space, SO2 can be used as a proxy of the presence of ash to anticipate air traffic issues caused by explosive eruptions. Moreover, volcanic SO2 strongly impacts air quality but also climate following its conversion to radiatively-active sulphate aerosols. However, the accurate assessment of these various impacts is currently hampered by the poor knowledge of volcanic SO2 emissions, which can substantially vary with time, in terms of flux and altitude. To fulfil this need, we propose a strategy relying on satellite observations, which consequently allows for monitoring the eruptive activity of any remote volcano. The method consists in assimilating snapshots of the SO2 load, provided every ~12 hours by IASI, in an inversion scheme that involves the use of a chemistry-transport model to describe the dispersion of SO2 released in the atmosphere. Applied on Eyjafjallajökull (Iceland) and Etna (Italy) eruption case-studies, this procedure allows for retrospectively reconstructing both the flux and altitude of the SO2 emissions with an hourly resolution. We show the improvement gained in the simulations and forecasts of the location and mass load of volcanic SO2 clouds using such a detailed reconstruction of emissions. For calibration-validation purpose, we compared our satellite-derived time-series of the SO2 flux with ground-based observations available on Etna. This comparison indicates a good agreement during ash-poor phases of the eruption. However, large discrepancies are observed during the ashrich paroxysmal phase as a result of enhanced plume opacity affecting ground-based ultraviolet spectroscopic retrievals. Therefore, the SO2 emission rate derived from the ground is underestimated by almost one order of magnitude. This result calls for the necessity to revisit currently available inventories of the global budget of sulfur released by volcanoes, because they heavily rely on groundbased observations. It also shows that volcano observatories cannot rely solely on ground-based spectroscopical observations for the monitoring of ash-rich explosive eruptions. Moreover, we will discuss the assimilation procedure of recently-developed IASI products which deliver snapshots of the volcanic SO2 cloud altitude. Such improvement renders the inversion procedure, used for the reconstruction of the altitude of emissions, independent of the wind shear prerequisite. Eventually, building on our accurate source of precursory SO2 gas emissions, we can explore the formation and lifecycle of sulphate aerosols in volcanic plumes. Remote sensing of tropospheric sulphate aerosols from moderate eruptions is not straightforward. However, we will show how a combination of chemistry-transport modelling and space-borne CALIOP lidar observations allows for tracking these aerosols despite their small concentration. The latest promising developments from high-resolution infrared sounders will bring further constraints on sulphate aerosol load and characteristics in dispersed volcanic clouds.
Complete list of metadatas

https://hal-insu.archives-ouvertes.fr/insu-01306362
Contributor : Catherine Cardon <>
Submitted on : Friday, April 22, 2016 - 8:33:55 PM
Last modification on : Sunday, July 21, 2019 - 6:40:50 AM

Identifiers

  • HAL Id : insu-01306362, version 1

Citation

Marie Boichu, Lieven Clarisse, Jean-Christophe Péré, Hervé Herbin, Philippe Goloub, et al.. Reconstruction of flux and altitude of volcanic SO2 emissions from IASI satellite observations: implications for volcanological and atmospherical studies.. 4th IASI International Conference, Apr 2016, Antibes Juan-Les-Pins, France. ⟨insu-01306362⟩

Share

Metrics

Record views

339