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ANTARCTIC OZONE
This page gives information about ozone at Halley, Rothera and Vernadsky/Faraday stations. It was either updated or new data was added on 2009 June 18.
The 2008 ozone hole season is over and the scene is being set for the 2009 season. Contrasts are increasing as the polar vortex builds with some circumpolar areas now above 370 DU and parts of the continent below 220 DU. Ozone levels generally remain below normal across the continent, though there are areas above normal in the circumpolar belt. The temperature of the ozone layer over Antarctica is cooling from the summer maximum, and an increasing area is now cold enough for polar stratospheric clouds (PSCs) to form. The ozone layer temperature remains generally a little below the normal.
The polar vortex was very stable throughout the season, and this governed the evolution of the 2008 ozone hole. During its initial stages, the ozone hole was much smaller than has been usual for August, but it grew rapidly as stratospheric clouds were exposed to sunlight. It covered over 25 million square kilometres in mid September, about the same as last year and remained at around 24 million square kilometres until early October. It shrank quite slowly, and persisted until the end of December, making it one of the longest lasting ozone holes on record. The vortex briefly showed a more elliptical circulation pattern at the end of October, and the ozone hole extended over the tip of South America, the Falkland Islands and South Georgia between October 28th and 30th. PSCs were seen from Rothera on several occasions and also at Halley.
See the final situation report for last year for information on the 2007 - 2008 season.
Notes: The Antarctic ozone hole is usually largest in early September and deepest in late September to early October. September 16 is world ozone day. 2007 was the International Year of the Ozone Layer. Prior to the formation of ozone holes, Antarctic ozone values were normally at their lowest in the autumn (ie March).
Click on a thumbnail to get the latest graph or high resolution image.
Halley - Total ozone: The ozone observation season started towards the end of August, and observations show that total ozone amounts fell at around 2 DU per day, from around 200 DU at the end of August (30% depletion) to around 125 DU (60% depletion) in late September. Values rose to reach 180 DU (45% depletion) in late October, but remained there until late November. From then they rose to reach 300 DU (10% depletion) in early January and had dropped to around 220 DU (25% depletion) by the end of the observing season in mid April. Superimposed on the general trends are small fluctuations with periods of days to around a month. The lowest daily value recorded was 118 DU on October 11. The December mean was the lowest on record for the month.
Rothera - Total ozone: Real-time
graphs showing current ozone and NO2 levels. Values were around 300
DU at the start of the year, then dropped a little, remaining at around 280 DU between mid January and mid
May. Ozone amounts rose from mid May until early July, reaching 320 DU.
From July values fell and reached 140 DU in early October. Daily
values initially rose rapidly in early October but then remained around
210 DU until late November. Values rose to 320 DU in early December, but
fell to 260 DU before rising rapidly at the end of the year. They
remained around 280 DU until early June, but have now risen to around 320 DU. Superimposed on
the general trends are fluctuations with periods of days to around a month and
values can change by over 50% in a few days as the polar vortex rotates across
the station. The lowest value
recorded was 118 DU on October 5. Note: The SAOZ instrument
constants were revised in July, and ozone values have been
increased by about 2% compared to previously published values.
Vernadsky - Total ozone: Vernadsky station is run by the National Antarctic Scientific Centre of Ukraine. Observations recommenced in late July and the preliminary results suggest that ozone levels dropped rapidly, and reached ozone hole levels in early August. They recovered to around 270 DU in mid August, but then dropped, reaching around 180 DU in early October (50% depletion). Values generally rose until mid November, and reached around 290 DU (25% depletion). Values then fell as the vortex extended over the station and reached 230 DU (40% depletion) towards the end of the month, before rising to 310 DU (15% depletion) in early December. Values fell to 260 DU (25% depletion) in late December before rising to 290 DU (15% depletion) in early January, and they remained near 280 DU (10% depletion) until the end of the observing season. Superimposed on the general trends are large fluctuations with periods of days to around a month, with daily values varying between 140 and 320 DU in the space of a few days. The lowest daily value reached was 134 DU on October 5.
Temperature and PSCs: The 100 hPa pressure level is near the base of the ozone layer, but is reached by most radiosonde flights. The temperature at this height is sufficiently cold from July to October that polar stratospheric clouds (PSCs) can form. The Antarctic stratosphere temperature is cooling, and in some areas is already cold enough for stratospheric clouds to form. Rothera saw this spectacular display of these clouds on 2007 July 12, and in 2008 saw them on June 3 (time lapse sequence taken by Rob Webster) and 30. Occasionally they are seen from Halley, and this year were seen on September 2.
Halley - 100 hPa temperature: The mean 100 hPa temperature at Halley
remained at winter temperatures of around -83°C until early October. It
rose, somewhat unsteadily, and peaked at -40°C in mid January, close to the
normal. The stratosphere is cooling and the 100 hPa
temperature has now dropped to -75°C, which is close to the
normal. The mean has remained below the normal since late August,
and the December mean was the coldest on record for the month.
Satellite: Satellite
imagery gives a global perspective on the ozone hole. Our
2008/2009 Antarctic ozone hole movie [updated
2009 May 6] is produced from OMI images, which are generally well calibrated
with respect to ground based measurements. The NCEP and KNMI analyses
are shown on the Canadian
Met Service daily ozone maps pages. In general the NCEP analysis in
the Southern Hemisphere tends to over-emphasise ozone depletion and the forecast
further increases the amount of depletion. The KNMI model is generally better at
analysis and forecasting in the Antarctic.
The SMOBA and TOAST analyses both use SBUV and TOVS data, but the TOAST algorithm
frequently over-estimates ozone depletion. US NWS CPC
plots from NOAA show the current
area of the ozone hole. The Sciamachy uv
index from the ESA Tropospheric Emission Monitoring Internet Service
shows the exposure risk at any location. Arctic:
Ozone values in the circumpolar belt built rapidly after the autumn minimum. An ozone depleted area, created by a combination of chemistry and dynamics,
was over the northern UK on December 26. A major, and unusually
early, spring warming took
place in late January and the stratospheric temperature became too warm for
stratospheric clouds to exist. After the warming, very high values, over
600 DU, were seen over some areas, before values began to drop.
Values across the Arctic and temperate parts of the
Northern Hemisphere now range from around 300 DU to above 400 DU. There are sometimes significant differences (over 100 DU) between modelled, satellite and
ground-based measurements. Ozone values over the
Arctic during 2008/9 are shown in our Northern Hemisphere TOMS movie. For more
UK information see the DEFRA UK
Stratospheric Ozone Measurements page. Equator: Ozone
levels are normally lowest over the topics and OMI data shows nothing unusual. Measurements reported here refer
to ozone in the "ozone layer", where most of the ozone in the atmosphere
is found. This "layer" stretches from roughly 10 to 40km above
the Earth's surface, with a peak at around 20km. Bringing all the ozone
in the "layer" down to ground level would give a thickness of around
3mm of pure ozone, which reduces to around 1mm at the height of the ozone hole.
A little ozone also exists closer to the Earth's surface and recent
research shows that natural halogens in Antarctica can produce depletion
in this near surface layer. The BAS ozone
bulletins contained the actual ozone values reported together with an analysis
of the situation. These were distributed by email on request, but are now superceded
by this web site. The last ozone bulletin
was issued on 2002 May 28. The final situation report
of each season is archived for historical reference. Please read this metadata
description before asking any questions about the data. [updated 2008 March 20].
Most of our data is available on line, however
please note that this is provisional and likely to change without warning.
You must request permission to reproduce
the data and I may be able to supply more suitable or more up to date material.
If data from Halley is used you must give the station name as Halley;
Halley Bay was a geographical feature that no longer exists. Provisional daily mean ozone
values for 2008/2009 for Halley
[Updated 2009 April 24] and Vernadsky. [Updated 2009 June 1] Temperature
and Ozone graphs for Halley and Vernadsky/Faraday. [Updated 2008 April 11].
The historic period shown in the inline graphs is for 1957 - 1972. Stratospheric Temperature
Rothera - Ozonesondes:
During 2003 we carried out ozone sonde flights at Rothera as part of the
QUOBI project. Data from these flights
is available in NASA-AMES format. Animation
of the ozonesonde flight results [note that although the ozone scale on these
graphs reads nanobars, it should read mPa]. Rothera - Ozone & nitrogen
dioxide: Some background information on Halley,
Rothera
and Faraday
stations is available from BAS. Information about Vernadsky station is also available
from the Ukrainian Antarctic Centre. Information about Vladimir Ivanovich
Vernadsky Some surface and upper air synoptic
data is also available on line from our public
data page. Southern Hemisphere ozone
hole movies for 1997/1998 , 1998/1999
, 1999/2000 , 2000/2001
, 2001/2002 , 2002/2003
, 2003/2004 , 2004/2005
, 2005 [TOMS], 2005/2006,
2006/2007, 2007/2008 and
2008/2009
[OMI, updated 2009 May 1]. A short sequence of the 2001
ozone hole. Requests for permission to use this data or for further
information should be sent to Jon Shanklin who maintains
these pages.
© Copyright Natural Environment Research Council - British Antarctic Survey
2009
Peninsula - 100 hPa temperature: The mean 100 hPa temperature in the
Antarctic Peninsula remained
at around -77°C
until early October,
significantly below the normal for this time of year (-74°C).
Values then slowly rose, with the final rapid spring warming occurring at the
end of November. The mean rose to -48°C in early December, a little below the normal of
-44°C, and then cooled to -51°C in late December. It peaked at -43°C in
mid January, close to the normal for this time of year, but has now fallen to
around -67°C, which is close to the normal for mid June. During the
spring there is often large day to day variation
because the area is in the
edge region of the circumpolar vortex.
Background and related material
Ozone bulletins
Ozone data
Provisional daily mean ozone values for Faraday/Vernadsky and Halley between 1972 and 2008. [Updated 2008 August 27]
Provisional monthly mean ozone values for Faraday/Vernadsky and Halley between 1956 and 2007.
Mean daily ozone values for the period 1957 - 1972 for Faraday
and Halley. [NB: not corrected to Bass-Pauer]
Daily ozone values for the period 1957 - 1973 for Faraday and Halley. [Revised to Bass-Pauer]
Monthly 100 hPa temperature means for The Antarctic Peninsula and Halley
between 1954 and 2008. [Updated 2008 May 7]
SAOZ total column nitrogen dioxide and ozone: 1996,
1997, 1998, 1999,
2000, 2001, 2002,
2003, 2004, 2005,
2006, 2007 and 2008
[to 2008 January 22].
"New" SAOZ total column nitrogen dioxide and ozone:
2006, 2007, 2008
and 2009
[updated 2009 June 18] and as real-time
graphs showing current ozone and NO2 levels.
Bentham ozone. Provisional values for 1997
/ 1998 / 1999 / 2000
/ 2001 / 2003 /
2004 [updated 2004 November 5 ].
Northern Hemisphere movies for 2000/2001 , 2001/2002
, 2002/2003 , 2003/2004
, 2004/2005 , 2005
[TOMS], 2005/2006, 2006/2007,
2007/2008 and 2008/2009 [OMI updated
2009 May 6]
A short sequence of ozone depletion during the 2002/03
northern winter showing the difference from the normal.
These annual movies are now about 4Mb and were compiled from daily TOMS images until the end of 2005; from
2005/06 they were compiled from OMI images. The movies begin and end in June.
Today's
OMI global image
The current
area of the hole and other
latest details are available from the NOAA Climate Prediction Center.
Environment Canada have an excellent set of daily
maps showing both northern and southern ozone levels from a variety of sources.
The Sciamachy uv index
from the ESA Tropospheric Emission Monitoring Internet Service.
Note that west longitude is negative when entering co-ordinates.
Contacts