Abstract

Abstract. Volcanic eruptions inject substantial amounts of halogens into the atmosphere. Chlorine and bromine oxides have frequently been observed in volcanic plumes from different instrumental platforms such as from ground, aircraft and satellites. The present study is the first observational evidence that iodine oxides are also emitted into the atmosphere during volcanic eruptions. Large column amounts of iodine monoxide, IO, are observed in satellite measurements following the major eruption of the Kasatochi volcano, Alaska, in 2008. The IO signal is detected in measurements made both by SCIAMACHY (Scanning Imaging Absorption Spectrometer for Atmospheric CHartographY) on ENVISAT (Environmental Satellite) and GOME-2 (Global Ozone Monitoring Experiment-2) on MetOp-A (Meteorological Operational Satellite A). Following the eruption on 7 August 2008, strongly elevated levels of IO slant columns of more than 4 × 1013 molec cm−2 are retrieved along the volcanic plume trajectories for several days. The retrieved IO columns from the different instruments are consistent, and the spatial distribution of the IO plume is similar to that of bromine monoxide, BrO. Details in the spatial distribution, however, differ between IO, BrO and sulfur dioxide, SO2. The column amounts of IO are approximately 1 order of magnitude smaller than those of BrO. Using the GOME-2A observations, the total mass of IO in the volcanic plume injected into the atmosphere from the eruption of Kasatochi on 7 August 2008, is determined to be on the order of 10 Mg.

Highlights

  • The IO signal is detected in measurements made both by SCIAMACHY (Scanning Imaging Absorption Spectrometer for Atmospheric CHartographY) on ENVISAT (Environmental Satellite) and GOME-2 (Global Ozone Monitoring Experiment-2) on MetOp-A (Meteorological Operational Satellite A)

  • Using the GOME-2A observations, the total mass of IO in the volcanic plume injected into the atmosphere from the eruption of Kasatochi on 7 August 2008, is determined to be on the order of 10 Mg

  • While on day August the volcanic plume is situated just in between two SCIAMACHY orbits, and only slightly enhanced amounts are seen at the edges of the plume in the adjacent orbits, the SCIAMACHY IO column amounts are largest on day August

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Summary

Introduction

A recent study by Saiz-Lopez et al (2015a) estimates that stratospheric iodine may range between 0.25– 0.7 pptv This is based on, for example, new aircraft observations in the tropics from which volume mixing ratios (VMRs) of IO between 0.1–0.2 pptv at altitudes up to 14 km were retrieved (Volkamer et al, 2015). For SCIAMACHY, the 3T retrieval was not successful (Schönhardt et al, 2008) due to instrumentrelated spectral features above 430 nm. It leads, to an improved quality of the IO retrievals from GOME-2A measurements. In terms of IO amounts, the results are consistent within the uncertainties between both GOME-2A retrievals as well as between GOME-2A and SCIAMACHY, cf. Sect. 3.2

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