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Non-linear quantization error reduction for the temperature measurement subsystem on-board LISA Pathfinder.
1Deutsches Zentrum für Luft- und Raumfahrt (DLR), Bremen 28359, Germany.
LISA Pathfinder mission data reveals analog-to-digital converter non-linearities degrade temperature sensor accuracy. A new post-processing method significantly reduces these errors, improving thermal noise measurements for future gravitational wave detectors.
Area of Science:
- Space physics and instrumentation
- Gravitational wave detection technology
- Precision measurement systems
Background:
- The Laser Interferometer Space Antenna (LISA) Pathfinder mission aims to validate technologies for space-based gravitational wave detection.
- Accurate measurement of thermal noise (∼10 μK Hz-1/2) is critical for validating LISA's noise models.
- Temperature sensors on LISA Pathfinder face performance degradation due to analog-to-digital converter non-linearities.
Purpose of the Study:
- To develop and validate a data post-processing method to mitigate analog-to-digital converter non-linearities in temperature measurements.
- To improve the accuracy of thermal noise monitoring for the LISA mission.
- To demonstrate the effectiveness of the proposed method using on-ground validation test data.
Main Methods:
- Implementing a novel data post-processing technique to correct for analog-to-digital converter non-linearities.
- Applying the method to experimental data from LISA Pathfinder's temperature measurement subsystem.
- Analyzing the noise reduction achieved in the sub-millihertz frequency range.
Main Results:
- The post-processing method effectively reduces the impact of analog-to-digital converter errors by a factor of three to six.
- An average noise reduction of 2.7 times was achieved in the 0.3 mHz-2 mHz frequency band.
- The method shows significant potential for improving in-flight data quality for LISA Pathfinder.
Conclusions:
- The developed post-processing technique successfully mitigates critical noise sources in temperature measurements.
- This advancement is crucial for validating noise models and ensuring the success of the future LISA mission.
- The findings demonstrate a viable approach to enhance precision measurements in space-based observatories.
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