Minimize MIPAS
Instrument image

The Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) MIPAS is a Fourier transform spectrometer for the detection of limb emission spectra in the middle and upper atmosphere. It observes a wide spectral interval throughout the mid infrared with high spectral resolution. Operating in a wavelength range from 4.15 microns to 14.6 microns, MIPAS detects and spectrally resolves a large number of emission features of atmospheric minor constituents playing a major role in atmospheric chemistry. Due to its spectral resolution capabilities and low-noise performance, the detected features can be spectroscopically identified and used as input to suitable algorithms for extracting atmospheric concentration profiles of a number of target species.

Status
Not Operational
Type
Atmospheric Chemistry and Temperature
Technical Characteristics
Accuracy:
Radiometric precision: 685-970cm-1: 1%, 2410 cm-1: 3%
Spatial Resolution:
Vertical resolution: 3km, vertical scan range 5-150km, Horizontal:3km x 30km, Spectral resolution: 0.035 lines/cm
Swath Width:
3 x 30 km
Waveband:
MWIR-TIR: between 4.15 and 14.6µm
Earth Topics
Atmosphere ( Ozone , Climate Change/Kyoto , Chemistry , Radiation/Temperature )
Related Instruments
Available Resources Type Access
Glossary Technical Document link
ENVISAT MIPAS An Instrument for Atmospheric Chemistry and ClimateResearch Special Publication order
MIPAS - An ENVISAT Instrument for Atmospheric Chemistry and ClimateResearch ESA Bulletin download
ACVE-3 Workshop Proceedings link
Annex A - Product Data Conventions Product Document download
MIPAS Products Specifications - NRT and Offline Processing Product Document download
MIPAS Products Specifications - Reprocessed dataset - info. preview Product Document download
Minimize Latest Mission Operations News

Envisat – MIPAS L1 dataset processed with MICAL v8.03 available online

22 January 2019

The Level 1 reprocessing of the full Envisat MIPAS mission with the ESA MICAL processor version 8.03 has been completed and the data has been assessed with respect to the quality. The reprocessed dataset is now accessible to users from the ESA dissemination server.