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TOTAL OZONE MONITORING BY GROUNDBASED INSTRUMENTS AS PART OF GAW. J. Staehelin 1 , R.Stübi 2 , U. Köhler 3 and A Redondas 4 1 Institute for Atmospheric and Climate Science, Swiss Federal Institute of Technology Zürich, Switzerland - PowerPoint PPT Presentation
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TOTAL OZONE MONITORING BY GROUNDBASED INSTRUMENTS
AS PART OF GAW J. Staehelin 1, R.Stübi 2, U. Köhler 3
and A Redondas 4
1 Institute for Atmospheric and Climate Science, Swiss Federal Institute of Technology Zürich, Switzerland
2 Federal Office of Meteorology and Climatology, MeteoSwiss, CH-1530 Payerne, Switzerland
3 Meteorological Observatory Hohenpeissenberg, Regional Dobson Calibration Centre RA VI, Albin-Schwaiger-Weg 10, D-82383
Hohenpeissenberg, Germany 4 Regional Brewer Calibration Center – Europe, Izaña Atmospheric Research
Center, AEMET- Meteorological State Agency, Spain, C/ La Marina 20, 6 Planta, 38071 Santa Cruz de Tenerife Spain
1. Introduction
CIMO guideChapter 17
Challenge:Total ozone series of Arosa
long-term changes: small
Outline
2. Instruments and method3. Dobson network4. Brewer network5. Experience with networks6. Future7. Conclusions
2. Instruments and methodoperated by MeteoSwiss at Arosa:
2 Dobson instruments 3 Brewer instruments (2 single and 1 double Brewer)
Dobson instrumentEarlier version: 1920th
method presently used: IGY: 1958
Brewer spectrophotometer commerc. available: middle of 1980th
completely automated, SO2 column, UV-B
Basic measurement principle (most precise measurements: direct sun)
Sun photometry, wavelength region: 305-340 nm
I (λ) = Io(λ) exp (-α(λ) X μ - β (λ) (ps/po) mR - δ (λ) ma)
X: total ozone amount (in Dobson units (DU)I (λ): solar irradiance at the wavelength λ measured at the Earth’s surface
Io (λ): intensity outside the Earth’s atmosphere
α(λ) is the monochromatic ozone absorption coefficient μ: relative slant path through ozone (air mass factor)
β(λ): Rayleigh scattering coefficientps: station pressure; po: mean sea level pressure at 1013.25 hPa;
mR: relative optical air mass corresp. to Rayleigh scattering (extinction)
δ(λ): aerosol optical depth ma: relative optical air mass corresp. to aerosol scattering (extinction)
Wavelengths used in Dobson (wavelength pairs (AD)) and Brewer instruments
(other Russian filter instruments and SAOZ (absorption in visible)
Calibration of instruments Io (λ): intensity outside the Earth’s atmosphere
• Extrapolation for = 0)Langley plot method
• Requirement: clean atmosphere and stable ozone for one half day
• Difficult to ensure in extratropics• Langley plot calibration for standard
instruments in Mauna Loa observatory (Hawaii)
3. Dobson network
Calibration of station instruments: Dobson intercomparisons (every 4 years) (Ulf Köhler): Responsibility of Regional Calibration Centers
Central CalibrationLaboratory: NOAA, Boulder, USA(R. Evans)
4. Brewer networkCentral Calibration Laboratory: Environment Canada, Toronto
(T. McElroy) : Triad: 3 Brewer instruments, regular Langley plot calibration of one instrument at Mauna Loa Observatory
European regional Brewer calibration center: Izaña (Tenerife) (A. Redondas): triad of Brewer spectrophotometers, regularly calibrated by the Langley plot method (redundancy in calibration scale)
Calibration of station instruments (every 2 years):• Canadian instruments: EC • for European instr.: European Brewer calibration center• Private companies (needs financing by stations)- IOS (International Ozone Service)- Kipp and Zonen (company producing Brewer instrument)
-1.0%
-0.5%
0.0%
0.5%
1.0%
1970 1975 1980 1985 1990 1995 2000 2005
1976 scale 1987 scale 1991 scale 1993 scale D065 Abs. Cal at MLO
Average Percent difference normalized to total ozone=300 DU, averaged over Mu=3, 2, 1
5. Experience with networks Dobson
Stability of calibration of World primary Dobson instrument (D083): Percent difference in calculated total ozone based on corrections to D083 A and D tables from Langley plot calibrations at Mauna Loa Observatory, Hawaii (Evans et al., 2004 and Komhyr et al., 1989).
Relative differences between standrad Dobson instruments and compared station instruments during initial calibrations of the
intercomparisons since 1969 (from Köhler et al., 2004).
Experience with network: Brewer
• Brewer instruments: More advanced technology (fully automated, more flexible)
• Different institutions involved in calibration of station instruments (private companies, need funding from stations)
• Biannual Brewer workshop: information of new developments, training of station personnel, exchange in experience
Comparison with satellite measurementsAbsolute and relative (in percent from the total number) number of sites with
‘‘no issues’’ (see text) in the record in 5 bins for Dobson, Brewer, and filter instrument sites located between 60oS and 60oN (from Fioletov et al., 2008).
0
20
40
60
80
100
1978-1985 1986-1990 1991-1995 1996-2000 2001-2006
0
10
20
30
40
50
60
1978-1985 1986-1990 1991-1995 1996-2000 2001-2006
Dobson Brewer Filter
Nu
mb
er o
f sta
tio
ns
6. Future
Ozone anomalies from model CMAM and measurements; Cly (Shepherd, 2008)
more ozone at lower stratosphere: greenhouse gas
7. Conclusions• For column ozone: two independent networks
operated under the auspices of GAW/WMO• Networks: high quality measurements (except
in polar regions at low solar elevation): suitable for long-term trend analysis and validation of satellite measurements
• Satellite instruments: limited life times, merged satellite series required for long-term trend analysis. High quality ground based networks need continuation !
Conclusions, cont.
• Ozone layer will recover from Ozone Depleting Substances (ODS, e.g. CFCs) (Montreal Protocol, 1987)
• Beneficial effect of Montreal Protocol on ozone layer by data analysis: controversial
• Demand for continuation of stratospheric ozone monitoring in future: Prediction of “super” recovery (more O3 in extratropical tropopause region): climate change
Acknowledgement: SAG-OzoneGeir Braathen (WMO) Johanna Tamminen (IGACO-O3/UV)
Frank Baier, Jack Fishman, Sophie Godin-Beekmann, Robert Evans1, Ulf Koehler12, Takeshi Koide12, Ed Hare, Tom McElroy2, Alberto Redondas2, Herman Smit, Rene Stübi12, Johannes Staehelin (chair), Richard Stolarski, Ronald van der A, Karel Vanicek12, Mark Weber
1: involved in Dobson measurements2: involved in Brewer measurements