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ABSTRACT

The atmosphere's ozone is concentrated in the so-called ozone layer. The atmosphere's ozone layer plays a very important role in protecting life on earth from potentially harmful UV rays, and it also helps shape the earth's climate. However, gasses resulting from human activity such as chlorofluorocarbons (CFC’s) are believed to deplete the ozone layer.

The discovery of a hole in the ozone layer which occurs each spring over Antarctica focused the world's attention on the importance of the ozone layer and stirred the global community into action.
Governments committed themselves to protecting the ozone layer and better understanding atmospheric processes.

Only satellites can measure ozone on a global scale, so they are essential for ozone studies. Satellite ozone data are mainly used for monitoring the global and vertical distribution of ozone, and are a valuable tool for policy makers who need to take appropriate measures to protect the ozone layer.

OBSERVATION AREA

SATELLITE DATA

ERBS: SAGE II
Nimbus-7, NOAA-9, -11, -12: SBUV
Nimbus-7, Meteor-3(5), TOMS-EP-94, ADEOS-I: TOMS
ERS2 GOME

Nadir viewing instruments perform measurements looking almost vertically beneath the satellite to the surface of the earth; as the satellite moves along its orbit, the instrument scans large bands on the earth surface. Such instruments measure the light of the sun (ultraviolet or infrared) that is reflected by the atmosphere and the earth’s surface. As light coming from the sun enters the atmosphere, it is partially absorbed and partially reflected back into space. The reflected part is analysed by the instrument on the satellite and special algorithms allow one to deduce the ozone content of the atmosphere and the vertical distribution of ozone in the stratosphere (ozone profile).

In the occultation technique, the satellite is positioned so that the earth progressively hides the light coming from the sun or a star as the satellite moves along its orbit. As the instrument sees the sun or star through the earth’s atmosphere, it can measure how the light is absorbed by the atmosphere at different altitudes. This method allows one to retrieve ozone profiles with a higher resolution in the stratosphere and the troposphere, but it has a much lower spatial and temporal coverage.

The SAGE II instrument is a seven-channel Sun photometer.
It yields 1-km vertical profiles of aerosols, ozone, nitrogen dioxide and water vapour. The focus of the measurements is on the lower and middle stratosphere, although retrieved aerosol, water vapour and ozone profiles often extend well into the troposphere under non-volcanic and cloud-free conditions.

The SBUV instrument directly measures the ultraviolet sunlight scattered by the Earth's atmosphere.
SBUV is a nadir-viewing instrument with a 200 kilometre square field of view. One measurement is made every 32 seconds along the orbital track, approximately every 1.8 degrees in latitude, from 80 degrees south to 80 degrees north. The Nimbus 7 spacecraft was in a south-to-north, sun-synchronous polar orbit so that it was always close to local noon/midnight below the spacecraft. Thus, ozone measurements were taken for the entire world every 24 hours.

The TOMS instrument measures total ozone by observing both incoming solar energy and backscattered ultraviolet (UV) radiation at six wavelengths.
TOMS is a nadir-viewing instrument and makes 35 measurements every 8 seconds, each covering an area 30 to 125 miles (50 to 200 kilometres) wide on the ground, strung along a line perpendicular to the motion of the satellite.

The GOME instrument is a nadir-scanning ultraviolet and visible spectrometer in the wavelength range 240-790 nm with a spectral resolution of 0.2 - 0.4 nm.
The satellite is on a sun-synchronous polar orbit and the instrument scans across-track with a field of view of 960 km divided into three 80x240-km pixels.

LINKS

On the British National Space Centre website

On the NASA Earth Observatory

On the Belgian Institute for Space Aeronomy website

On Eduspace