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What is ozone?

What is ozone?. O 3 a very reactive molecule consisting of 3 oxygen atoms strong oxidant reacts easily by ”giving” one of its oxygen atoms to another molecule. Where do we find ozone?. in the stratosphere (ca 10 - 50 km) absorbing harmful UV-radiation in the troposphere (ground level)

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What is ozone?

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  1. What is ozone? • O3 • a very reactive molecule • consisting of 3 oxygen atoms • strong oxidant • reacts easily by ”giving” one of its oxygen atoms to another molecule

  2. Where do we find ozone? • in the stratosphere (ca 10 - 50 km) • absorbing harmful UV-radiation • in the troposphere (ground level) • as a pollutant • part of photochemical smog • damage on vegetation/crops • damage on respiratory system • produced by electrical discharges • as naturally by lightnings • in useful applications • as desinfecting agent (e.g. for purifying water) • because of its oxidizing effect

  3. What is the ozone layer? • part of the stratosphere (from ca 15-35 km) that is enriched in ozone • but even there the concentrations are very low (between 1 – 20 ppm) • the altitude varies with the latitude, with the seasons and the time of the day

  4. Measuring unit for ozone • Dobson unit (DU) • 100 DU = 1 mm ozone thickness at STP (1 atm, 0ºC) • typical values: 300 – 500 DU • if ozone was compressed to pressure at sealevel it would have a thickness of 3 – 5 mm • if the whole atmosphere was compressed to sealevel pressure it would have a thickness of ca 8 km

  5. Measuring ozone (1) • satellites • ground measurements • balloons • aircrafts • rockets

  6. Measuring ozone (2) • satellites • usually passive instruments that use solar radiation • most instruments register only total ozone • example: TOMS (Total Ozone Mapping Spectrometer) • uses Backscatter Ultraviolet Technique: • 2 measurement (pair measurements) for each used wavelength in the UV-range: • (1) radiation directly from the sun • (2) radiation that is reflected from the ground or backscattered from the atmosphere • measurements at at least 2 different wavelength, one absorbing weakly, one absorbing strongly • changes in the pair measurements for these wavelength are used to calculate ozone amount • for the strong absorbing wavelength: the more ozone, the less is reflected/backscattered

  7. Measuring ozone (3) • ground measurements • passive instruments (Dobson) • measurements of UV-radiation from the sun at 2 wavelength, one strongly absorbed, one weakly absorbed (similar to the backscatter technique on satellites) • other atmospheric phenomenons (clouds, aerosols ….) affect both wavelength in the same way, • the remaining difference between the wavelength is due to ozone. • active instruments (LIDAR) • LIDAR = Light Detection and Ranging • laserlight is used in the same way as radiowaves in a RADAR • beams of two wavelength of UV-light are emitted from a laser • one strongly absorbed by ozone, the other weakly • the reflected/backscattered fotons are measured for both wavelengths • calculations in a similar way as for backscattering method on satellites and the Dobson-instrument • with LIDAR one can also get an ozone profile, not only total ozone • measurements can be done during darkness

  8. Measuring ozone (4) • balloons • in situ measurements (directly measuring the ozone in a sample) • often used: chemical reactions • balloons burst at 30 – 35 km altitude • no data of the highest part of the ozone layer (but above 30 km there is little ozone) • airplanes and rockets(less used than the other platforms) • in situ measurements • (big rockets and planes in the stratosphere are believed to contribute to the destruction of the ozone layer • scientists do not agree on the degree of destruction)

  9. Variations of ozone • Most ozone is produced in the stratosphere above the equator • The highest ozone level is at higher latitude • transportation from the equator • little annual variation in ozone concentration over the equator • about 25% annual variation at higher latitudes • reasons for natural variations: • seasons, suncycle, winds

  10. Annual global ozone variations Source: www.ofcm.gov/jagti/11-03_mtg/long_uviI_jag-it.ppt

  11. How and where is ozone created? • O2+hf  O + O UV-radiation • O2 + O  O3 • in the stratosphere • mainly over the equator • where the UV-radiation is most intense

  12. How is ozone destructed? • Physical processes • O3+hf  O + O2 UV-radiation • O3 + O  2O2 • Chemical processes • O3+RRO + O2 RO + O R + O2 O3+ O  2O2 net reaction • R: free radicals • reactive compounds with an unpaired electron • function as catalysts in the ozone destruction reaction • R: NO, NO2, HO, Cl or Br … • Cl and Br are liberated from e.g. CFC and halons by UV-radiation

  13. How does the Arctic ozone ”hole” develop? 3 necessary conditions: • (1) development of a polar vertex during winter • strong winds around the pole inhibit exchange with air outside the vertex •  no supply of ozone • (2) low temperatures  ice crystals develop • formation of polar stratospheric clouds • ice particles catalyse ozone destruction • with nitric acid (HNO3) ice formation occurs at higher temperatures (ca -80º C) • (3) UV-radiation (sunlight) supplies energy to break down e.g. CFC and halones • formation of more reactive compounds (free radicals) • especially of Cl and Br from CFC and halons  The ozone hole develops just after the sun returns during spring.

  14. Ozone profile from day to day over the South Pole in 2003 Source: http://www.cmdl.noaa.gov/ozwv/ozsondes/spo/ozone_anim2003.html

  15. Amount of UV-radiation on the ground How much UV-radiation we are exposed to depends on: • the total amount of ozone • angle to the sun • latitude • time of the year • time of the day • elevation • cloud cover • aerosols

  16. ERYTHEMAL UV-EXPOSURE • is the energy from UV-radiation that an area on the ground receives during a given period of time • unit: • watt/squaremeter or • joule/squaremeter (measured over the hours with most intense UV-radiation) • this gives an indication of the risk for sunburn

  17. Risks of a low ozone level • higher risk for skin cancer • higher risk for eye diseases • higher risk of DNA damage in organisms • effect on plants vary • some grow better • but e.g. soya grows less (could mean reduced harvest/food) • not enough knowledge to predict exact effect on plankton • some species die at high UV-rates • this effect would propagate through the food chain • others assimilates at higher rates  disturbance of the balance in ecological systems

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