total ozone surface climate characteristics GMD Annual Meeting, - - PowerPoint PPT Presentation

total ozone surface climate characteristics
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total ozone surface climate characteristics GMD Annual Meeting, - - PowerPoint PPT Presentation

total ozone surface climate characteristics GMD Annual Meeting, Boulder, May 21./22., 2013 With the peak of EESC concentrations reached in the late 1990s, can a recovery in ozone be detected over Antarctica already? Are there


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SLIDE 1

GMD Annual Meeting, Boulder, May 21./22., 2013

total ozone surface climate characteristics

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SLIDE 2

GMD Annual Meeting, Boulder, May 21./22., 2013

  • With the peak of EESC

concentrations reached in the late 1990s, can a recovery in ozone be detected over Antarctica already?

  • Are there dynamical changes that

affect ozone concentrations?

  • If there are dynamical changes, do

they also affect Antarctic surface characteristics, like sea ice extend?

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SLIDE 3

GMD Annual Meeting, Boulder, May 21./22., 2013 Southpole Syowa Halley Faraday/ Vernadsky total column ozone

  • zone sondes

both

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SLIDE 4

GMD Annual Meeting, Boulder, May 21./22., 2013 Southpole Syowa Halley Faraday/ Vernadsky total column ozone

  • zone sondes

both

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SLIDE 5

GMD Annual Meeting, Boulder, May 21./22., 2013 Southpole Syowa Halley Faraday/ Vernadsky total column ozone

  • zone sondes

both

Lat: -65.3° Lat: -69.0° Lat: -75.5° Lat: -90.0°

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SLIDE 6

GMD Annual Meeting, Boulder, May 21./22., 2013

  • 1. Vortex breaks up earlier
  • 2. Not as much ozone depletion

due to lower concentrations of EESC

  • 3. Vortex gets smaller
  • 4. Change in vortex location
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SLIDE 7

GMD Annual Meeting, Boulder, May 21./22., 2013

  • 1. Vortex breaks up earlier
  • 2. Not as much ozone depletion

due to lower concentrations of EESC

  • 3. Vortex gets smaller
  • 4. Change in vortex location
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SLIDE 8

GMD Annual Meeting, Boulder, May 21./22., 2013

  • Change in equivalent latitude of

vortex edge with time:

  • For 550 K

( .: area enclosed by same PV contour, placed circular around the pole  resulting latitude)

  • NCEP/NCAR reanalysis (PV)
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SLIDE 9

GMD Annual Meeting, Boulder, May 21./22., 2013

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SLIDE 10

GMD Annual Meeting, Boulder, May 21./22., 2013 Southpole Syowa Halley Faraday/ Vernadsky total column ozone

  • zone sondes

both c

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SLIDE 11

GMD Annual Meeting, Boulder, May 21./22., 2013

MSU TLS

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SLIDE 12

GMD Annual Meeting, Boulder, May 21./22., 2013

Location of vortex changed over time, moving eastward

  • Heterogeneous chemistry still

plays major role for Antarctic ozone concentrations in spring

  • When looking for ozone recovery, it

is important to clearly separate between dynamically and non- dynamically influenced ozone values

 Hassler et al., GRL 2011

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SLIDE 13

GMD Annual Meeting, Boulder, May 21./22., 2013

  • Is it possible to find impacts of this

strong stratospheric temperature signal in Antarctic surface parameters, e.g. sea ice extent?

  • What is cause and what is effect?
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SLIDE 14

GMD Annual Meeting, Boulder, May 21./22., 2013

1979 – 2009, MSU TLS

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SLIDE 15

GMD Annual Meeting, Boulder, May 21./22., 2013

1979 – 2009

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SLIDE 16

GMD Annual Meeting, Boulder, May 21./22., 2013

1979 – 2009

Holland & Kwok, Nat. Geosci 2012

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SLIDE 17

GMD Annual Meeting, Boulder, May 21./22., 2013

  • A connection between Antarctic vortex

temperatures and Antarctic sea ice extent might exist

  • Shift in October vortex position might

be reflected in summer/fall sea ice extent, however:

  • High uncertainties still on signal due

to more influence factors on data

  • Cause and effect still unclear