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SIFTI
Static Infrared Fourier Transform Interferometer
INSTRUMENT 
SIFTI is a Fourier Transform interferometer with no moving mirror
SIFTI provides spectra of the infrared radiance emitted by the Earth in the ozone and CO band
Lifetime: 3 to 5 years

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The project main steps

Timeline

 

Measuring ozone and carbon monoxide concentrations in the boundary layer of the atmosphere (the atmospheric layer near the surface, between 0 and 3 km roughly) is a major challenge for air quality. Infrared sounding, providing profiles with information at several vertical levels, is a must for pollution monitoring.

In this framework, CNES is currently leading a phase-A study for the instrument SIFTI, Static Infrared Fourier Transform Interferometer, devoted to ozone and CO measurements. In the TRAQ proposal to the ESA Earth Explorer mission, SIFTI could be associated with two other instruments: TROPOMI, a UV-VIS spectro-imager and OCAPI, a multi-angle polarised spectro-radiometer based on the Polder or Parasol heritage.


Latest Update 09/02/2009
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NEWS
March 10th, 2009
GST meeting in Paris CNES Headquarters
 
January 20th-21st, 2009
ESA Earth Explorer user consultation meeting
 
October 20th, 2008
GST meeting in Paris CNES Headquarters
 
September, 2008
New publications
 
June 20th, 2008
GST meeting in Paris CNES Headquarters
 
May 2008
SIFTI poster at International TOVS study Conference XVI