MIPAS on ENVISAT
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The Michelson
Interferometer for Passive Atmospheric Sounding (MIPAS)
is an high resolution Fourier Transform Spectrometer developed by ESA
for the detection of limb emission spectra in the upper atmosphere.
MIPAS has been successfully launched on board Envisat-1, on 1 st
March
2002. It detects the atmospheric limb emission over a wide spectral
interval in the middle infrared region.
Up to now MIPAS mission can be divided in 3 parts:
- measurements from June 2002 to March 2004
- measurements on August - September 2004
- measurements from January 2005 on
The characteristics of the instrument that are common to the different
periods of measurements are summarised in the
following table:
Type
|
Parameters |
Pointing
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Instantaneous
Field of View |
3 x 30 km2
(height per width,
at 10 km tangent altitude) |
Elevation
pointing |
5 ... 210 km
(tangent altitude)
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Spectral
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Spectral
range
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685-970 cm-1,
1020-1170 cm-1, 1215-1500 cm-1, 1570-1750 cm-1,
and 1820-2410 cm-1
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Radiometric
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Radiometric
sensitivity NESR
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50, 40, 20, 6 and
4.2 nW/cm2/sr/cm-1, respectively for the above
spectral ranges
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The characteristics distinguishing the measurements in the different
periods are the spectral resolution and the # of spectra per standard
elevation scan.
The measured middle
infrared emission spectra contain features of most
atmospheric constituents. Therefore, a series of spectra measured in
the limb-scanning configuration can be processed to determine the
volume mixing ratio profiles of numerous atmospheric trace species.
The retrieval of pressure and temperature, as well as the volume mixing
ratio of six high priority species, namely O 3, H 2O,
HNO 3, CH 4, N 2O and
NO 2, are routinely performed in near real time.
Official Site: http://envisat.esa.int/instruments/mipas/
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