Abstract

Abstract. We use satellite-borne measurements collected over the last decade (2006–2015) from the Aura Microwave Limb Sounder (MLS) and the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) to investigate the nitric acid distribution and the properties of polar stratospheric clouds (PSCs) in the early winter Antarctic vortex. Frequently, at the very start of the winter, we find that synoptic-scale depletion of HNO3 can be detected in the inner vortex before the first lidar detection of geophysically associated PSCs. The generation of "sub-visible" PSCs can be explained as arising from the development of a solid particle population with low number densities and large particle sizes. Assumed to be composed of nitric acid trihydrate (NAT), the sub-visible PSCs form at ambient temperatures well above the ice frost point, but also above the temperature at which supercooled ternary solution (STS) grows out of the background supercooled binary solution (SBS) distribution. The temperature regime of their formation, inferred from the simultaneous uptake of ambient HNO3 into NAT and their Lagrangian temperature histories, is at a depression of a few kelvin with respect to the NAT existence threshold, TNAT. Therefore, their nucleation requires a considerable supersaturation of HNO3 over NAT, and is consistent with a recently described heterogeneous nucleation process on solid foreign nuclei immersed in liquid aerosol. We make a detailed investigation of the comparative limits of detection of PSCs and the resulting sequestration of HNO3 imposed by lidar, mid-infrared, and microwave techniques. We find that the temperature history of air parcels, in addition to the local ambient temperature, is an important factor in the relative frequency of formation of liquid/solid PSCs. We conclude that the initiation of NAT nucleation and the subsequent development of large NAT particles capable of sedimentation and denitrification in the early winter do not emanate from an ice-seeding process. Finally, we investigate the patterns of interannual variability and compare the relative formation frequency of liquid and solid PSCs in the Antarctic lower polar stratosphere using the results of a cluster analysis to synthesize the combined CALIOP and MLS measurements into a relatively small number of interrelated categories.

Highlights

  • In Lambert et al (2012) we reported on the formation of polar stratospheric clouds (PSCs) and the initial stages of denitrification in the early 2008 Antarctic PSC season

  • We have selected some views from the combined Microwave Limb Sounder (MLS) and Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) data record to illustrate how the interpretation of the morphology of PSCs and gas-phase HNO3 in along-track transects is governed by the local ambient temperature, and by the underlying temperature histories

  • We developed a compact visual representation of the daily orbit tracks that allows a time series to be constructed from the montage of a few hundred separate daily images, consisting of a combination of different days/pressure levels/species, and displayed on a single page

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Summary

Introduction

In Lambert et al (2012) we reported on the formation of polar stratospheric clouds (PSCs) and the initial stages of denitrification in the early 2008 Antarctic PSC season. In order to resolve discrepancies involving implied condensed HNO3 above that available from the gas phase (including additional HNO3 brought down by renitrification) and growth/sedimentation rates that are not commensurate with back-trajectories, those authors hypothesized that the particles are non-compact or highly aspherical or NAT-coated ice. Grooß et al (2014) coupled a saturation-dependent parameterization of the ZOMM heterogeneous NAT scheme with the Chemical Lagrangian Model of the Stratosphere (CLaMS) and determined that derived PSC properties were in better agreement with CALIOP data than for simulations using a constant rate NAT nucleation, confirming the results of Hoyle et al (2013). 5 the early stages of formation of Antarctic PSCs at 68–21 hPa in 2009 are examined using CALIOP PSC types and Lagrangian temperature history, with the inference of an initial population of subvisible solid-particle NAT clouds superseded by a predominantly liquid STS composition over a period of about a week.

Datasets and methodology
CALIOP PSC data
MLS gas-phase constituents
Temperature history and relation to NAT nucleation and growth processes
Visual representation of satellite orbital data
Detection and classification of PSCs
Equilibrium STS
Intercomparisons of PSC detection techniques
Evaluation of CALIOP and MLS co-located measurements
MLS and CALIOP orbit transects
Denitrification and renitrification
Time series of PSC formation and Lagrangian temperature history
Interannual variations in the early Antarctic PSC season
Conclusions
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