Sensitivity of temperature retrieval in the Martian atmosphere to transmittance simulation accuracy and instrumental noise

Details Sensitivity of temperature retrieval in the Martian atmosphere to transmittance simulation accuracy and instrumental noise Sensitivity of temperature retrieval in the Martian atmosphere to transmittance simulation accuracy and instrumental noise

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000p%26ss...48..473h&link_type=abstract

Planetary and Space Science, Volume 48, Issue 5, p. 473-481.

Computer Science

1

Scientific paper

The Mars-Express mission in 2003 will carry the Planetary Fourier Spectrometer (PFS) for measurement of infrared radiation emitted by the atmosphere and surface. The retrieval of vertical temperature profiles is based on an iterative comparison of measured and simulated spectra in the 15 μm CO2 band. A sensitivity study is performed to define the required accuracy of line-by-line CO2 transmittance simulations to obtain reliable temperature results. The influence of instrumental noise on the temperature retrieval is also discussed. Synthetic measurements as well as selected spectra from the Mariner 9-IRIS data were used in the study.

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