MOLI instrument -for MOtionLess Interferometertakes advantage of the new concept of static Fourier transform spectrometer. It is a high-resolution spectrometer working over a narrow bandwidth, which is adapted to a wide range of atmospheric sounding missions and compatible with micro-satellite platform The core of this instrument is an echelette cube. Mirrors on the classical design are replaced by stepped mirrors -integrated into that interference cube- thus suppressing any moving part. The steps' directions being set over a perpendicular axis, the overlap of both stepped mirrors creates a cluster of so-called "echelettes", each one corresponding to a different optical path difference (OPD). Hence the Fourier transform of the incoming radiance is directly imaged on a CCD array in a single acquisition. The frequency domain of the measurements is selected by an interferential filter disposed on the incoming optical path. A rotating wheel equipped with several filters allows the successive measurement of spectra around some bands of interest, i.e. O 2, CO2 and CO absorption bands. Climate change, CO 2 monitoring, Static Fourier Transform spectrometer, Echelette cube, Green-house effect.
CITATION STYLE
Rosak, A., & Tintó, F. (2004). Progress report of a static fourier transform spectrometer breadboard. In European Space Agency, (Special Publication) ESA SP (pp. 67–71). https://doi.org/10.1117/12.2307973
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