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Elastic Particle Swarm Optimization for MarSCoDe Spectral Calibration on Tianwen-1 Mars Rover
Xiong Wan1,2,3, Rujun Yuan3, Hongpeng Wang2,3
1Key Laboratory of Systems Health Science of Zhejiang Province, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China.
A new elastic particle swarm optimization (PSO) method corrects spectral shifts and line mismatches for the MarSCoDe instrument on China's Tianwen-1 Mars rover. This advanced calibration ensures accurate mineral analysis despite extreme Martian temperature fluctuations.
Area of Science:
- Planetary Science
- Spectroscopy
- Robotics Engineering
Background:
- China's Tianwen-1 Mars rover utilizes the MarSCoDe laser-induced breakdown spectroscopy (LIBS) instrument for mineral and rock analysis.
- MarSCoDe faces extreme temperature variations (approx. 100 °C range) on Mars, causing significant spectral shifts and calibration line inconsistencies.
Purpose of the Study:
- To develop and validate an on-board spectral calibration method for MarSCoDe capable of handling harsh Martian environmental conditions.
- To address spectral shifts and spectral line number mismatches caused by temperature fluctuations and environmental changes.
Main Methods:
- An elastic particle swarm optimization (PSO) algorithm was employed for spectral calibration.
- A standard wavelength set (SWS) and particle wavelength sets (PWS) were established, with elastic selection from PWS for comparison with SWS.
- Testing was conducted using standard lamps and a Titanium (Ti) target within a Mars simulation environment chamber (MSEC) across a 70 °C temperature range.
Main Results:
- The PSO approach effectively corrected spectral shifts, reducing them to within 0.015 nm.
- A specific spectral line shift of 8.09 nm was corrected to approximately 0 nm.
- The method successfully addressed both spectral shift and spectral line number mismatch issues.
Conclusions:
- The elastic PSO-based approach provides robust on-board spectral calibration for MarSCoDe under challenging Martian conditions.
- This method enhances the accuracy of mineral and rock composition analysis by the rover.
- The technique is adaptable for calibrating other spectral payloads in deep space exploration missions.
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