ACE-FTS
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "ACE-FTS".

The Canadian SCISAT spacecraft during testing at the Canadian Space Agency David Florida Laboratory (DFL) in Kanata, Ontario.

SCISAT-1 is a Canadian satellite designed to make observations of the Earth's atmosphere. Its most important instrument is an optical Fourier transform infrared spectrometer, the ACE-FTS Instrument. This device records the spectrum of the Sun, as sunlight passes through the Earth's atmosphere, and makes an analysis of the chemical elements of the atmosphere possible.

SCISAT is a relatively small satellite weighing 150 kg (~330 pounds). It is partly drum shaped with a diameter of about five feet and a depth of about five feet. The Canadian Space Agency coordinated its design, launch and use. The main contractors were Bristol Aerospace of Winnipeg, Manitoba and ABB Bomem inc. of Quebec City, Quebec.

SCISAT passes through the Earth's shadow 15 times per day, profiting from the occultation of the Sun to make a spectrographic analysis of the structure and chemistry of those parts of the upper atmosphere that are too high to be reached by balloons and airplanes and too low to be visited by orbiting satellites. This kind of analysis can help understand the depletion of the ozone layer and other upper atmosphere phenomena.

SCISAT was placed in low Earth orbit, or LEO, by a Pegasus rocket launched from a carrier aircraft on August 12, 2003. It is expected to operate for two to five years.

The University of Waterloo, York University, the University of Toronto, and several other Canadian universities collaborated in the design of the experiments, and in several aspects of the testing of the satellite.

ACE-FTS

The ACE-FTS instrument is the main payload of the SCISAT-1 spacecraft. The primary scientific goal of the Atmospheric Chemistry Experiment (ACE) is to measure and understand the chemical and dynamical processes that control the distribution of ozone in the upper troposphere and stratosphere. The principle of ACE measurement is the solar occultation technique. A high inclination (74 degrees), low earth orbit (650 km/400 miles) will provide ACE coverage of tropical, mid-latitudes and polar regions.

The spectrometer is an adapted version of the classical Michelson interferometer using an optimized optical layout. Its highly folded double-pass optical design results in a very high performance instrument with a compact size. A signal-to-noise ratio (SNR) better than 100 is achieved, with a field-of-view (FOV) of 1.25 mrad and an aperture diameter of 100 mm (4"). A semiconductor laser is used as the metrology source of the interferometer sub-system.

The auxiliary Visible/Near-infrared Imager (VNI) monitors aerosols based on the extinction of solar radiation using two filtered detectors at 0.525 and 1.02 micrometres. The instrument also includes a suntracker mechanism providing fine pointing toward the radiometric center of the sun with stability better than 3 μrad. The ACE-FTS instrument was launched on August 12, 2003.

ABB was the prime contractor for the design and manufacturing of the ACE-FTS instrument.

External Links

• The Atmospheric Chemistry Experiment (ACE)
• [1] ABB Bomem inc.