1 / 17

Assessment of the Stratospheric Ozone Layer: Past and Future (Karma of and Nirvana for O 3 )

Assessment of the Stratospheric Ozone Layer: Past and Future (Karma of and Nirvana for O 3 ). A.R. (Ravi) Ravishankara NOAA, Earth System Research Laboratory Chemical Sciences Division. What were the major findings from the 2006/2007 assessment

eydie
Télécharger la présentation

Assessment of the Stratospheric Ozone Layer: Past and Future (Karma of and Nirvana for O 3 )

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Assessment of the Stratospheric Ozone Layer: Past and Future (Karma of and Nirvana for O3) A.R. (Ravi) Ravishankara NOAA, Earth System Research Laboratory Chemical Sciences Division What were the major findings from the 2006/2007 assessment Where were some of the big issues/uncertainties My personal take on what are likely to be the big issues in the next assessment and beyond No discussion of organizational issues in this talk - a little premature Color code: Black or red- What the assessment said Blue- What I think (possibly wrongly!)

  2. Updating the Ozone Assessment Science Assessment of Ozone Depletion: 2006 Many of you contributed directly and all contributed indirectly Cochairs Ayité-Lô Ajavon (Togo) Daniel L. Albritton (USA) Robert T. Watson (USA) Scientific Steering Committee Marie-Lise Chanin, CNRS, France Susana Diaz, CAIC, Argentina John Pyle, University of Cambridge, UK Theodore Shepherd, University of Toronto, Canada A. R. Ravishankara, NOAA, USA

  3. The 2006 Science Assessment • Incremental, but significant, changes/updates • The Parties took some key action in Montreal based on this assessment • - HCFCs will be phased out sooner • The coupling to climate is a major issue 1989 1991 1994 1998 2002 2006

  4. The Preparation of the 2006 Science Assessment, con’t • The Terms of Reference from the Parties (Decision XV/53): • Assess the state of the ozone layer and its expected recovery • Discuss recent occurrences of the Antarctic ozone hole • Evaluate trends in ozone-depleting substances (ODSs) • Analyze the role of atmospheric bromine in ozone depletion • Assess the impacts of climate change on the ozone layer’s recovery • Discuss past trends and future expectations for global ozone, polar ozone, and surface ultraviolet radiation Questions for the “accountability” phase of the Montreal Protocol

  5. The Major Findings and Conclusions of the 2006 Science Assessment ODS production ODS production (a) (b) (c) (d) Ozone-depleting chlorine and bromine in the stratosphere ODS in the atmosphere Ozone levels – measured and predicted Global ozone change Ultraviolet radiation change UV levels – measured and predicted 1980 Now~ 2100 Work of many as viewed from way up there… The Montreal Protocol is working! (Ozone improving? Influence on UV, climate, etc.?)

  6. Issues of Production of Ozone-DepletingSubstances This is what the countries (people) care about a lot… Important Issue! chlorofluorocarbons hydrochlorofluorocarbons ODSproduction CFCs HCFCs – less efficient than CFCs, but still destroys ozone CFCs are still produced by Article 5 countries 1980 Now ~ 2100 • HCFCs will continue to contribute to ozone depletion until • roughly the middle of the 21st century. (Impact of last week’s decision in Montreal?!) • Release of “banked” CFCs (and Halons) will also contribute. Can the productions be translated to emissions and emissions to atmospheric abundances? Reporting of emissions/production in the past and in the future…

  7. Trends of Ozone-Depleting Substances in the Atmosphere • ODS decreasing in the lower atmosphere (where they are emitted) as well as in the stratosphere where the ozone layer is • MP is working as intended in terms decreases in ODSs ODS Changes in the stratosphere ODS Changes in the lower atmosphere

  8. Ozone-depleting chlorine and bromine in the stratosphere 1980 Now~ 2100 Trends of Ozone-Depleting Chemicals in the Atmosphere: The Future Combined effective abundances of ozone-depleting chlorine and bromine in the stratosphere. • Uncertainties in transport, banks, and future emissions lead to uncertainties in future levels. • Failure to continue compliance with the MP could delay, or even prevent, the ozone layer recovery.

  9. Issues about Trends of Ozone-Depleting Chemicals in the Atmosphere • How does the EESC change with time? • - Chlorine-bromine mix? Future emissions? • - Transport (climate change?) • Dealing with Lifetime issues • - Age of air issues: in the past, now and the future • Short-lived species have contributed a lot to current decline… • - Transport of the short-lived and very short-lived species species (t < a couple of weeks, e.g., CF3I) are important… • Concept and quantification of “lifetime” • For both long-lived and short-lived gases • Implication to metrics! (ODP, GWP)

  10. ? 2010 Global Ozone Observations • There are early signs that the ozone layer is starting its expected recovery. • A clear statement on recovery would “require” having a clear temporal trend in ozone AND Attribution of changes to all contributors… Coupling and non-linearity…

  11. Polar Ozone Changes Polar O3 loss remains large and highly variable, as measured by many metrics. • The annual variations are expected in the next decades. • Variations in the ozone hole during this and next decade are mostly due to meteorology – ozone hole in 2002 and 2006 are not “anomalous.” • The duration of the ozone hole will change the extent of “ozone hole” & Arctic ozone depletion in the future. • Impact of climate change and compositional change on ozone hole.

  12. Explaining the Past and Predicting the Future Global ozone change 1980 Now~ 2100 Models Observations • Based on ODS abundances and modeling calculations, estimates of “recovery to pre-1980 value” are now: ~ 2050 at mid-latitudes (better estimates of the “banks” of ODSs) ~ 2065 for the Antarctic ozone hole (age of air) ~2050 for the Arctic springtime ozone depletions • Volcanoes can influence ozone levels, but only for a few years This is a complex issue with non-linear dependencies… Is this treated adequately? Appropriately? People care about these dates! (& they are often misunderstood!)

  13. Reality? Reality? Model “Recovery”: What is it? • Return of the ozone layer to pre-1980 values (when it was not significantly influenced by ODS) is considered “recovery”. • Multiple factors contribute to the return of ozone to pre-1980 values. Climate change and ODS will affect the future of ozone layer. Concept

  14. “Recovery”: A big issue Return of the ozone layer to pre-1980 values (when it was not significantly influenced by ODS) is considered “recovery”. • An operational definition? A better definition? Do we need a definition? Is it a good concept? • “Beyond” natural variability? Would the variability get larger? Smaller? • Is 1980 a good “baseline?” - chemically, dynamically? Other factors (e.g., solar cycle)? Do we talk about “super or sub recovery?” • Is it essential that all models agree? Is explaining the past essential for predicting the future?

  15. “Recovery”: A big issue, contd. Multiple factors contribute to the return of ozone to pre-1980 values. Climate change and ODS will affect the future of ozone layer. • Other factors? • The contributions of “polar ozone depletions” on mid-latitude ozone. • What are the vertical distributions of the ozone layer changes? • Is the Upper Strat the best place to look for effect of ODSs? Decreases in ODS emissions already achieved by MP is the dominant factor in ozone returning towards its pre-1980 values- • At least in the next couple of decades.. Later in the century? • Difficulties in attribution when changes are smaller…

  16. Explaining the Past and Predicting theFuture: UV Ultraviolet radiation change 1980 Now ~ 2100 • Basic understanding of variation in UV with ozone remains unchanged. • Large global ozone depletions in a world without MP would have led to very large UV increases. UV changes will not be a major driver Impacts of stratospheric ozone changes on climate and the troposphere (weather, predictability, etc.) are the emerging issues

  17. Thank you for your attention

More Related