Abstract

Abstract. The long-term stratospheric impacts due to emissions of CO2, CH4, N2O, and ozone depleting substances (ODSs) are investigated using an updated version of the Goddard two-dimensional (2-D) model. Perturbation simulations with the ODSs, CO2, CH4, and N2O varied individually are performed to isolate the relative roles of these gases in driving stratospheric changes over the 1850–2100 time period. We also show comparisons with observations and the Goddard Earth Observing System chemistry-climate model simulations for the time period 1960–2100 to illustrate that the 2-D model captures the basic processes responsible for long-term stratospheric change. The ODSs, CO2, CH4, and N2O impact ozone via several mechanisms. ODS and N2O loading decrease stratospheric ozone via the increases in atmospheric halogen and odd nitrogen species, respectively. CO2 loading impacts ozone by: (1) cooling the stratosphere which increases ozone via the reduction in the ozone chemical loss rates, and (2) accelerating the Brewer-Dobson circulation (BDC) which redistributes ozone in the lower stratosphere. The net result of CO2 loading is an increase in global ozone in the total column and upper stratosphere. CH4 loading impacts ozone by: (1) increasing atmospheric H2O and the odd hydrogen species which decreases ozone via the enhanced HOx-ozone loss rates; (2) increasing the H2O cooling of the middle atmosphere which reduces the ozone chemical loss rates, partially offsetting the enhanced HOx-ozone loss; (3) converting active to reservoir chlorine via the reaction CH4+Cl→HCl+CH3 which leads to more ozone; and (4) increasing the NOx-ozone production in the troposphere. The net result of CH4 loading is an ozone decrease above 40–45 km, and an increase below 40–45 km and in the total column. The 2-D simulations indicate that prior to 1940, the ozone increases due to CO2 and CH4 loading outpace the ozone losses due to increasing N2O and carbon tetrachloride (CCl4) emissions, so that total column and upper stratospheric global ozone reach broad maxima during the 1920s–1930s. This precedes the significant ozone depletion during ~1960–2050 driven by the ODS loading. During the latter half of the 21st century as ODS emissions diminish, CO2, N2O, and CH4 loading will all have significant impacts on global total ozone based on the Intergovernmental Panel on Climate Change (IPCC) A1B (medium) scenario, with CO2 having the largest individual effect. Sensitivity tests illustrate that due to the strong chemical interaction between methane and chlorine, the CH4 impact on total ozone becomes significantly more positive with larger ODS loading. The model simulations also show that changes in stratospheric temperature, BDC, and age of air during 1850–2100 are controlled mainly by the CO2 and ODS loading. The simulated acceleration of the BDC causes the global average age of air above 22 km to decrease by ~1 yr from 1860–2100. The photochemical lifetimes of N2O, CFCl3, CF2Cl2, and CCl4 decrease by 11–13 % during 1960–2100 due to the acceleration of the BDC, with much smaller lifetime changes (<4 %) caused by changes in the photochemical loss rates.

Highlights

  • Changes in the atmospheric abundance of halogenated ozone depleting substances (ODSs) and the greenhouse gases (GHGs) CO2, CH4, and N2O have been shown to significantly impact the chemical and dynamical structure of the stratosphere (e.g., World Meteorological Organization (WMO), 2007, 2011)

  • We have used an updated version of our Goddard Space Flight Center (GSFC) 2-D coupled model to study long-term stratospheric changes caused by source gas loading for the 250-yr time period, 1850–2100

  • We compare the 2-D simulations with global ozone and temperature changes observed during the recent past, and with simulations from the Goddard Earth Observing System chemistryclimate model (GEOSCCM)

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Summary

Introduction

Changes in the atmospheric abundance of halogenated ozone depleting substances (ODSs) and the greenhouse gases (GHGs) CO2, CH4, and N2O have been shown to significantly impact the chemical and dynamical structure of the stratosphere (e.g., World Meteorological Organization (WMO), 2007, 2011). Detection of the change in the halogen influence on ozone can be complicated by the impacts due to long-term changes in GHGs. It is of interest to separate the relative impacts of the different chemical processes that control longterm ozone changes. Some 3-D CCM investigations have shown the impact of different processes on long-term stratospheric change, such as that due to the multi-decadal changes in ODS and GHG concentrations and sea surface temperatures (SSTs) (e.g., Butchart and Scaife, 2001; Austin et al, 2007; Olsen et al, 2007; Li et al, 2008; Eyring et al, 2010a, b; Austin et al, 2010). In this paper we expand on these previous studies and examine in more detail the relative contributions of the longterm changes in atmospheric GHG and ODS loading using our recently upgraded Goddard Space Flight Center (GSFC) 2-D coupled chemistry-radiation-dynamics model. The good 2-D model agreement with the measurements and the GEOSCCM justifies the use of the 2-D model for the perturbations addressed in this study

Model simulations
Quantification of the ozone impacts due to GHGs
Summary and conclusions
Wave parameterizations
Radiative transfer
Tropospheric parameterizations
Temperature
Findings
N2O and H2O

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