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Calibration of MAJIS (Moons And Jupiter Imaging Spectrometer). III. Spectral calibration
Paolo Haffoud1, François Poulet1, Mathieu Vincendon1
1Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.
The Moons And Jupiter Imaging Spectrometer (MAJIS) underwent extensive calibration to define its spectral performance. On-ground and in-flight data confirm MAJIS meets its mission requirements for exploring Jupiter's icy moons.
Area of Science:
- Planetary Science
- Space Instrumentation
- Spectroscopy
Background:
- The Moons And Jupiter Imaging Spectrometer (MAJIS) is crucial for ESA's Jupiter Icy Moons Explorer mission.
- Pre-flight calibration is essential for characterizing instrument performance and identifying distortions.
Purpose of the Study:
- To present analyses of on-ground and in-flight datasets for MAJIS.
- To characterize the spectral performances of the MAJIS instrument.
- To compare derived performances against mission requirements.
Main Methods:
- Conducted two on-ground calibration campaigns at the instrument level.
- Acquired in-flight measurements during the Near-Earth Commissioning Phase.
- Analyzed spectral calibration data using monochromatic and polychromatic sources with various samples.
Main Results:
- Derived spectral sampling and spectral response functions across the entire field of view.
- Quantified spectral characteristics considering operational parameters like temperature and spectral binning.
- Compared on-ground derived performances with in-flight measurements.
Conclusions:
- MAJIS's spectral performance has been thoroughly characterized using both ground and in-flight data.
- The instrument's spectral characteristics meet the established performance requirements for the mission.
- This calibration ensures the reliability of MAJIS data for exploring Jupiter's icy moons.
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