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Calibration of MAJIS (Moons And Jupiter Imaging Spectrometer). II. Spatial calibration.
Gianrico Filacchione1, Paolo Haffoud2, Francois Poulet2
1INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00133 Rome, Italy.
The Review of Scientific Instruments
|April 23, 2024
Summary
The Moons and Jupiter Imaging Spectrometer (MAJIS) instrument
Area of Science:
- Planetary Science
- Astrophysics
- Space Instrumentation
Background:
- The Jupiter Icy Moons Explorer (JUICE) mission aims to study Jupiter's icy moons.
- The Moons and Jupiter Imaging Spectrometer (MAJIS) is a key instrument for this mission.
- Pre-flight characterization and calibration are crucial for ensuring instrument performance.
Purpose of the Study:
- To thoroughly measure and document the spatial responses of the MAJIS instrument before its space mission.
- To assess how instrument performance varies across its field of view and operational temperature range.
- To establish a baseline for comparing pre-flight and in-flight instrument behavior.
Main Methods:
- Detailed measurements of spatial response functions (slit, pixel, knife edge, ensquared energy, keystone aberration).
- Testing across multiple field of view positions and relevant temperature ranges.
- Description of experimental setups and data analysis methodologies.
Main Results:
- Comprehensive dataset of MAJIS spatial responses obtained under various conditions and wavelengths.
- Characterization of instrumental aberrations and functions.
- Identification of minor changes in instrument response and channel coalignment post-launch by comparing with initial in-flight data.
Conclusions:
- The pre-flight calibration campaign provided a detailed understanding of MAJIS's spatial response.
- Post-launch data revealed slight deviations from ground measurements, necessitating in-flight monitoring.
- These findings are vital for accurate data interpretation from the JUICE mission.
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