Sources and Impacts of Short-Lived Anthropogenic Chlorine

Lead Research Organisation: University of Leeds
Department Name: School of Earth and Environment

Abstract

Depletion of stratospheric ozone allows larger doses of harmful solar UV radiation to reach the surface leading to increases in skin cancer and cataracts in humans and other impacts, such as crop damage. Ozone also affects the Earth's radiation balance and, in particular, ozone depletion in the lower stratosphere (LS) exerts an important climate forcing. While most long-lived ozone-depleting substances (e.g. CFCs) are now controlled by the United Nations Montreal Protocol and their abundances are slowly declining, there remains significant uncertainty surrounding the rate of ozone layer recovery. Changes in the LS may cause delayed ozone recovery or even additional depletion, and can also have important effects on climate. One key uncertainty, highlighted in the WMO/UNEP 2014 Assessment of Stratospheric Ozone Depletion, is the increasing importance of uncontrolled chlorine-containing very short-lived substances (VSLS) which can reach the LS and cause ozone depletion.

While significant amounts of brominated VSLS are known to be emitted naturally from the oceans, recent publications also show a rapid, unexpected and unexplained increase in anthropogenic chlorinated VSLS (Cl-VSLS), especially in E and SE Asia. Some of these Cl-VSLS will reach the stratosphere via deep convection in the tropics (through the tropical tropopause layer) or via the Asian Summer Monsoon (ASM) or the E Asian Winter Monsoon.

The Montreal Protocol is arguably the world's most successful environmental agreement. By controlling the production and emission of long-lived ODSs, it has set the ozone layer on the road to recovery. However, short-lived halogenated compounds (lifetimes <6 months) have so far not been included, based on the belief that they would not be abundant or persistent enough to have an impact. Recent observations suggest otherwise; calculations in this proposal suggest that Cl-VSLS may delay the recovery of the Antarctic Ozone Hole (to 1980 levels) by up to 30 years. Fortunately, the Montreal Protocol has a regular review process which allows amendments to deal with new threats to the ozone layer and climate, e.g. the recent 2016 success of including limits to the production of hydrofluorocarbons (HFCs).

This proposal takes advantage of UEA's heritage in atmospheric halocarbon measurements to obtain novel observations of chlorine compounds in the key E/SE Asia region and in the global mid-upper troposphere. Surface observations will be targeted in the key winter periods when we know that we will be able to detect polluted emissions from China, a likely major emitter of Cl-VSLS globally. We will extend the suite of gases currently measured by the CARIBIC in-service global passenger aircraft to include several newly-identified VSLS. This will allow us to investigate the distribution of these VSLS over a much wider geographical area, to identify source regions and to assess longer term changes in their atmospheric abundance.

Our observations will be combined with detailed 3-D modelling at Leeds and Lancaster, who have world-leading expertise and tools for the study of atmospheric chlorine. One model will be used in an 'inverse' mode to trace back the observations of anthropogenic VSLS to their source regions. Overall, the models will be used to quantify the flux of halogenated ozone-depleting gases to the stratosphere and to determine their ozone and climate impact. We will calculate metrics for ozone depletion and climate change and feed these through to the policy-making process (Montreal Protocol) with the collaboration of expert partners. The results of SISLAC will provide important information for future international assessments e.g. WMO/UNEP and IPCC reports.

Planned Impact

We anticipate that the halocarbon dataset generated from the proposed work will feature heavily in future WMO/UNEP Stratospheric Ozone Assessments, particularly when assessing the impact of the Asian region on global emissions and when evaluating the role of very short-lived substances (VSLS) on stratospheric ozone. This will be a continuation of the impact of the halocarbon research programmes at UEA and ULeeds over the past 20 years, who have been regular contributors to international assessments, including the last five of the quadrennial WMO/UNEP Stratospheric Ozone Assessments and various reports to the IPCC. In addition to having our data and model calculations regularly included in these assessments, we have further contributed as lead authors, co-authors, contributors and reviewers. Chipperfield (PI) is now on the steering committee for the 2018 WMO/UNEP Assessment. One of the case studies in the UEA 2014 submission to REF was focussed on this activity and the School of Environmental Sciences came 1st for Impact in the Earth Sciences category.

Although written primarily by scientists, the WMO and IPCC reports are aimed very much at policy makers and, to a lesser extent, a more general audience, through the co-publication of additional material such as the Summary for Policy Makers. The reports are also made available online.

We believe there will also be a strong interest in our findings from the chlorocarbon production industry, particularly in view of the potential for chlorinated VSLS to be included in the Montreal Protocol, which would have a very large impact on the sector. With this in mind we have made arrangements with representatives of the halocarbon producers and policy advisors to exchange information on current industrial practice and interests surrounding the issue of chlorinated VSLS and the Montreal Protocol. These include David Sherry, who is a consultant with expertise in the chlorocarbon industry, and Stephen Anderson, who is a long-term advisor to the Parties of the Montreal Protocol (see Letters of Support). In return we will provide industry with current tropospheric abundance data and estimates of "top-down" regional and global emissions. These can be compared with industry calculated "bottom-up" emissions which are based on production and sales figures. Furthermore, we will calculate new ozone depletion potentials (ODPs) for chlorinated VSLS which are used directly to formulate policy. (Calculation of ODPs for short-lived species is not straightforward and requires realistic understanding of their sources and atmospheric fate which we will obtain in SISLAC). We anticipate that there will be pressure on policymakers over the coming years to consider adding compounds such as dichloromethane to the list of compounds restricted by the Montreal Protocol. Through the above means, SISLAC will contribute towards evidence-based policy making at both national and international levels.

SISLAC as a whole will lead to an improved representation of VSLS emissions in the Asian monsoon region in global chemistry/climate and earth system models. This in turn will improve current understanding as to the significance of the monsoon in topics including stratospheric ozone depletion and future ozone recovery, and associated future climate impacts/prediction (issues which have a large impact on society). This will benefit parties involved in climate prediction.

Publications

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Chipperfield M (2020) Renewed and emerging concerns over the production and emission of ozone-depleting substances in Nature Reviews Earth & Environment

 
Description That so far short-lived chlorine species have not caused major stratospheric ozone depletion, although they have the potential to in the future.

The recently discovered, illegal production of CFC-11 has the potential to delay ozone layer recovery. However, if swift action is taken, this delay could be small (small compared to natural variability). Recent data shows that the CFC-11 emissions decreased strongly after 2018.
Exploitation Route To support the Montreal Protocol process - to strengthen current implementation and to include new species.
Sectors Chemicals

Environment

 
Description Results fed into the 2018 and 2022 WMO/UNEP Stratospheric Ozone Assessments. This is the process which supports the Montreal Protocol to avoid emissions of gases that deplete the ozone layer. Results were also used for the 2021 Special Report into CFC-11 Emissions.
First Year Of Impact 2018
Sector Environment
Impact Types Policy & public services

 
Description Lead Author WMO/UNEP Ozone Assessment 2022
Geographic Reach Multiple continents/international 
Policy Influence Type Participation in a guidance/advisory committee
Impact Input to the Montreal Protocol on substances which protect the ozone layer.
 
Description Montreal Protocol Scientific Assessment Steering Committee
Geographic Reach Multiple continents/international 
Policy Influence Type Membership of a guideline committee
Impact Reduction in stratospheric ozone depletion and in surface climate change
 
Description Why is Lower Stratospheric Ozone Not Recovering?
Amount £649,267 (GBP)
Funding ID NE/V011863/1 
Organisation Natural Environment Research Council 
Sector Public
Country United Kingdom
Start 01/2022 
End 06/2025
 
Title Data used in: 'Atmospheric impacts of chlorinated very short-lived substances over the recent past - Part 1: Stratospheric chlorine budget and the role of transport' by Bednarz et al. (2022) 
Description Data used in: 'Atmospheric impacts of chlorinated very short-lived substances over the recent past - Part 1: Stratospheric chlorine budget and the role of transport' by Bednarz et al. (2022), which has been accepted for publication in Atmospheric Chemistry and Physics. 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
URL https://zenodo.org/record/6993692
 
Title Intital simulation of Hunga-Tonga volcanic aerosol cloud with the UM-UKCA composition-climate model 
Description This dataset is from a series of "forward projection" interactive stratospheric aerosol simulations of the Jan 2022 Hunga-Tonga volcanic aerosol cloud with the UM-UKCA composition-climate model. The model experiments predict how the cloud will disperse through 2022, and apply the UM-UKCA model at GA4 (Walters et al., 2014), with GLOMAP v8.2, as applied for the "MajorVolc" datasets for Agung, El Chichon and Pinatubo (Dhomse et al., 2020), those runs aligned with the Historical Eruption SO2 emissions Assessment experiment within ISA-MIP (Timmreck et al., 2018). The "standard" Hunga-Tonga GA4 UM-UKCA experiment emits 0.4Tg of SO2 at 29-31km, within a 24-hour period, matching the detrainment duration specified for the ISA-MIP HErSEA experiment protocol. Following the stronger than expected mid-visible backscatter ratios (BSR) measured by CALIOP satellite-borne lidar, and from ground-based lidar from Reunion Island (very high BSR values > 200), we also ran UM-UKCA simulations with "scaled-up Hunga-Tonga SO2 emission", at 0.8, 1.2 and 1.6 Tg of SO2 emitted. Unexpectedly strong stratospheric AOD observed from the OMPS satellite months after the eruption further strengthens the motivation for these simulations. Several hypotheses for the high AOD from Hunga-Tonga have been suggested: 1) an unusual amount of (or influence from) co-emitted ultra-fine ash particles 2) "in-plume oxidised sulphate" already converted from SO2 at the time of detrainment (e.g. via aqueous-phase oxidation within water droplets within the eruptive plume). 3) co-emitted marine aerosol (e.g. sea-salt aerosol) from seawater vaporized in the plume There are 4 types of netcdf files, Stratospheric AOD (saod), Effective Radius (reff), Extinction (ext) and sulphate aerosol surface area density (sad). For e.g. saod550_HT_0pt4Tg_T2Mz-20220101-20230831.nc contains Stratospheric aerosol optical depth (sAOD) at 550nm (2D-monthly dataset vs latitude and time) with 0.4 Tg SO2 injection Jan2022 to August 2023 Whereas other files reff_HT_0pt4Tg_T2Mz_20220101-20230831.nc, sad_HT_0pt4Tg_T2Mz_20220101-20230831.nc ext550_HT_0pt4Tg_T2Mz-20220101-20230831.nc contain particle effective radius (reff), aerosol surface area density, aerosol extinction as 3D-monthly fields (altitude, latitude , time) from the same simulation. Other saod and extinction files are also available at 870 and 1020 nm. Note that these are preliminary simulations, hence we do not expect good match with the observations. We plan to perform additional UM-UKCA simulations, comparing to the satellite and ground-based lidar measurements, and to in-situ balloon observations from Reunion Island rapid response campaign & upcoming high-altitude balloon sampling flights in Brazil. References : Dhomse SS, Mann GW, Antuña Marrero JC, Shallcross SE, Chipperfield MP, Carslaw KS, Marshall L, Abraham NL, Johnson CE. 2020. Evaluating the simulated radiative forcings, aerosol properties, and stratospheric warmings from the 1963 Mt Agung, 1982 El Chichón, and 1991 Mt Pinatubo volcanic aerosol clouds. Atmospheric Chemistry and Physics. 20(21), pp. 13627-13654 Timmreck, C., Mann, G. W., Aquila, V., Hommel, R., Lee, L. A., Schmidt, A., Brühl, C., Carn, S., Chin, M., Dhomse, S. S., Diehl, T., English, J. M., Mills, M. J., Neely, R., Sheng, J., Toohey, M., and Weisenstein, D.: The Interactive Stratospheric Aerosol Model Intercomparison Project (ISA-MIP): motivation and experimental design, Geosci. Model Dev., 11, 25812608, https://doi.org/10.5194/gmd-11-2581-2018, 2018. 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
URL https://zenodo.org/record/6621919
 
Title TCOM-HCl : Daily global gap-free stratospheric hydrogen chloride profile data set based on TOMCAT CTM and Occultation Measurements 
Description Methodology: TOMCAT simulation is performed at T64L32 resolution for the 1991-2021 time period. Collocated hydrogen chloride (HCl) profiles are divided in five latitude bins: SH polar (90S-50S), SH mid-lat (70S-20S), tropics (40S-40N), NH mid-lat (20N-70N) and NH polar (50N-90N). Initially, model-measurement differences are calculated for each zonal bins (46 height levels, 15km to 60km). Separate XGBoost regression models are trained for the differences between TOMCAT and measurements at each level for a given latitude bin. XGBoost model is then used to estimate error corrections for all the TOMCAT grids ( day/night, 2 X11323 time steps). TOMCAT output sampled at 1.30 am and 1.30 pm local time at the equator. Estimated corrections for a given model grid that are added to the original TOMCAT simulated day and night time HCl profiles. Height resolved data are then interpolated on 28-pressure levels (300 - 0.1hPa). For overlapping latitude bins, we use averages and then calculate daily zonal mean values. For more details see attached presentation. Dataset also includes two files containing daily mean zonal mean HCl profiles on height (15-60 km) and pressure (300-0.1 hPa) levels: zmhcl_TCOM_hlev_T2Dz_1991_2021.nc - height level data (15 to 60 km) zmhcl_TCOM_plev_T2Dz_1991_2021.nc - pressure level data (300 to 0.1 hPa) Daily 3D profiles on height and pressure levels would be made available upon request 
Type Of Material Database/Collection of data 
Year Produced 2023 
Provided To Others? Yes  
URL https://zenodo.org/record/7608193
 
Title TCOM-HF : Daily global gap-free stratospheric hydrogen fluoride (HF) profile data set based on TOMCAT CTM and Occultation Measurements 
Description Methodology: TOMCAT simulation is performed at T64L32 resolution for the 1991-2021 time period. Collocated hydrogen fluoride (HF) profiles are divided in five latitude bins: SH polar (90S-50S), SH mid-lat (70S-20S), tropics (40S-40N), NH mid-lat (20N-70N) and NH polar (50N-90N). Initially, model-measurement differences are calculated for each zonal bins (46 height levels, 15km to 60km). Separate XGBoost regression models are trained for the differences between TOMCAT and measurements at each level for a given latitude bin. XGBoost model is then used to estimate error corrections for all the TOMCAT grids ( day/night, 2 X11323 time steps). TOMCAT output sampled at 1.30 am and 1.30 pm local time at the equator. Estimated corrections for a given model grid that are added to the original TOMCAT simulated day and night time hydrogen fluoride profiles. Height resolved data are then interpolated on 28-pressure levels (300 - 0.1hPa). For overlapping latitude bins, we use averages and then calculate daily zonal mean values. For more details see attached presentation. Dataset also includes two files containing daily mean zonal mean hydrogen fluoride profiles on height (15-60 km) and pressure (300-0.1 hPa) levels: zmhf_TCOM_hlev_T2Dz_1991_2021.nc - height level data (15 to 60 km) zmhf_TCOM_plev_T2Dz_1991_2021.nc - pressure level data (300 to 0.1 hPa) Daily 3D profiles on height and pressure levels would be made available on request. 
Type Of Material Database/Collection of data 
Year Produced 2023 
Provided To Others? Yes  
URL https://zenodo.org/record/7607563
 
Title TOMCAT CTM simulated ozone profiles using NRL2, SATIRE and SORCE solar fluxes 
Description Individual file contain TOMCAT CTM simulated ozone profiles from five model simulations analysed in the following publication. Briefly, vmro3_T2Mz_TOMCAT_A_NRL2_2005-2020.nc contain ozone profiles from the control simulation that uses ERA5 dynamical forcing fields and NRL V2 solar fluxes vmro3_T2Mz_TOMCAT_B_SATIRE_2005-2020.nc and vmro3_T2Mz_TOMCAT_C_SORCE_2005-2020.nc contain ozone profiles from a simulations that are similar to the control simulation but with SATIRE and SORCE solar fluxes vmro3_T2Mz_TOMCAT_D_SFix_2005-2020.nc has ozone profiles from simulation that is similar to the control simulation but with fixed solar fluxes, whereas vmro3_T2Mz_TOMCAT_E_DFix_2005-2020.nc also contain ozone profiles from a simulation where model uses annually repeating dynamical fields. Dhomse, S. S., Chipperfield, M. P., Feng, W., Hossaini, R., Mann, G. W., Santee, M. L., and Weber, M.: A Single-Peak-Structured Solar Cycle Signal in Stratospheric Ozone based on Microwave Limb Sounder Observations and Model Simulations, Atmos. Chem. Phys. Discuss. [preprint], https://doi.org/10.5194/acp-2021-663, in review, 2021. 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
URL https://zenodo.org/record/5875189