1 longitudinally-dependent ozone recovery in the antarctic polar vortex revealed by...
TRANSCRIPT
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Longitudinally-dependent ozone recovery Longitudinally-dependent ozone recovery in in the Antarctic polar vortex revealed by the Antarctic polar vortex revealed by
satellite-onboard ILAS-II observation in 2003satellite-onboard ILAS-II observation in 2003
Kaoru SatoDepartment of Earth and Planetary Science
The University of Tokyo, Tokyo, Japan
*Yoshihiro TomikawaNational Institute of Polar Research, Tokyo, Japan
H. Nakajima, and T. SugitaNational Institute for Environmental Studies, Ibaraki, Japan
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Stratospheric transport and mixing processes related to the ozone recovery
Holton et al.
(Rev. Geophys, 1995)
Purposes of this study to examine• What is three dimensional structure of the ozone recovery?• Is the B-D circulation only the process contributing ozone
recovery before the polar vortex breaking?
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Antarctic ozone hole and its observations in 2003
Ozonesonde observations at Syowa Station O3 data from 97 ECC ozonesondes for 11 June 2003 – 9 January 2004
ILAS-II (Improved Limb Atmospheric Spectrometer-II) observations
O3 and long-lived tracers (N2O and CH4) in the stratosphere at 14 longitudes a day for 15 June –25 October 2003.
The Antarctic ozone hole in 2003 was developed into large (3rd after 2000 and 2006) and showed a similar life cycle to that in 2000.
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Time variation of O3 partial pressure
Vertical profiles of O3 partial pressure at Syowa Station (69S, 39.6E) (left) from late June to early October and (right) from early October to early December.
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Seasonal variation of the polar vortex in the Antarctic in 2003
Tangential wind speeds along the potential vorticity contours at 500K (colors). Contours show the potential vorticity (PVU).
500K 19 20kmz
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Seasonal variation of O3 mixing ratio at Syowa Station
Time-height section of O3 mixing ratio from ozonesonde observations at
Syowa Station (69S, 39.6E). Thick dashed curves show the -80oC isotherms roughly indicating possible PSC areas.
1.1±0.2 km/mon
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Seasonal variation of O3 mixing ratio
as a function of longitudeobserved by ILAS-II
•The downward movement of the
contour in late September through late
October is clear in any longitude region.
•An interesting feature is that the
downward speed is largely dependent on
longitude.
Time-height sections of O3 mixing ratio (colors) inside the polar vortex for six longitude regions based on the ILAS-II observations. Contours show isentropic surfaces.
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Descent rates (km/mon) as a function of longitude
▲: N2O X : CH4●: O3 : *w―
Descent rates around z=20km estimated using ILAS-II observations. Right marks show the zonal means.
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Dynamical fields in 25 Sep.-24 Oct., 2003
Maps of (a) the time mean geopotential height and (b) its anomaly from the zonal mean at 50 hPa (z~20km). Time series of (c) GPH amplitude and (d) temperature as a function of longitude.
Schematic view of longitudinally-dependent descent rate. Black lines represent isentropes. Red arrows show descent rates.
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Decent rates around relative to the isentrope estimated from ILAS-II observations.
Descent rates (K/mon) as a function of longitude
▲: N2O X : CH4●: O3
500K
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Backward trajectory analysis
Backward trajectories starting at (a) 0-60oE and (b) 180-240oE shown by blue shades.
A map of total ozone averaged for 26 Sep. to 24 Oct. 2003.
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Time variation of scatter diagrams of O3 and N2O
Scatter diagrams of O3 and N2O mixing ratios for every ten days. Different colors show results at different isentropic levels.
ozon
e
N2O
vortex inside
vortex outsidemixing line
.0)O/NO/(N
,0)/O/(O
,0O/N and 0/O Since
.0ON,0O induces Mixing
22ON
33O
23
23
2
3
zδwδ
zδwδ
zz
δδ
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Conclusions
• Three dimensional nature of the ozone recovery processes in the
Antarctic spring was examined based on ozonesonde and satellite
observations.
• The ozone recovery was largely dependent on longitude in
isentropic coordinates even before the polar vortex breaking.
• This feature is explained by trajectories of air parcels which are
largely modified by dominant quasi-stationary planetary waves.
• Strong mixing with ozone rich air at the polar vortex edge seems
to occur for air parcels observed in particular longitude regions.