Abstract

Abstract. In this work, a novel approach for the determination of the particle size distribution (PSD) parameters of stratospheric sulfate aerosols is presented. For this, ratios of extinction coefficients obtained from SAGE III/ISS (Stratospheric Aerosol and Gas Experiment III on the International Space Station) solar occultation measurements at 449, 756 and 1544 nm were used to retrieve the mode width and median radius of a size distribution assumed to be monomodal lognormal. The estimated errors at the peak of the stratospheric aerosol layer, on average, lie between 20 % and 25 % for the median radius and 5 % and 7 % for the mode width. The results are consistent in magnitude with other retrieval results from the literature, but a robust comparison is difficult, mainly because of differences in temporal and spatial coverage. Other quantities like number density and effective radius were also calculated. A major advantage of the described method over other retrieval techniques is that both the median radius and the mode width can be retrieved simultaneously, without having to assume one of them. This is possible due to the broad wavelength spectrum covered by the SAGE III/ISS measurements. Also, the presented method – being based on the analysis of three wavelengths – allows unique solutions for the retrieval of PSD parameters for almost all of the observed extinction spectra, which is not the case when using only two spectral channels. In addition, the extinction coefficients from SAGE III/ISS solar occultation measurements, on which the retrieval is based, are calculated without a priori assumptions about the PSD. For those reasons, the data produced with the presented retrieval technique may be a valuable contribution for a better understanding of the variability of stratospheric aerosol size distributions, e.g. after volcanic eruptions. While this study focuses on describing the retrieval method, and a future study will discuss the PSD parameter data set produced in depth, some exemplary results for background conditions in June 2017 are shown.

Highlights

  • The existence of a permanent aerosol layer in the stratosphere, typically known as the Junge layer, has been known about since the late 1950s when Christian Junge performed balloon-borne in situ measurements there (Junge et al, 1961)

  • Ratios of extinction coefficients obtained from SAGE III/ISS (Stratospheric Aerosol and Gas Experiment III on the International Space Station) solar occultation measurements at 449, 756 and 1544 nm were used to retrieve the mode width and median radius of a size distribution assumed to be monomodal lognormal

  • While this study focuses on describing the retrieval method, and a future study will discuss the particle size distribution (PSD) parameter data set produced in depth, some exemplary results for background conditions in June 2017 are shown

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Summary

Introduction

The existence of a permanent aerosol layer in the stratosphere, typically known as the Junge layer, has been known about since the late 1950s when Christian Junge performed balloon-borne in situ measurements there (Junge et al, 1961). Anthropogenic SO2 emissions play a role in the variation of the stratospheric aerosol (SA) budget (Sheng et al, 2014), but they are dwarfed by natural sources, especially by direct injections due to large volcanic eruptions. Intense biomass burning events, such as the Canadian wildfires in 2017 (Ansmann et al, 2018) and the Australian bushfires of 2019– 2020 (Ohneiser et al, 2020), can play an important role in the feeding of the aerosol layer. The Junge layer is persistent globally over time, even in volcanically quiescent periods and without large biomass burning events (Kremser et al, 2016). The stratospheric aerosol layer is mainly sustained by a flux of sulfurous aerosols and precursor gases from the troposphere, such as SO2 and OCS

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