Results 191 to 200 of about 10,414 (210)
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Tilt-to-length coupling and diffraction aspects in satellite interferometry
2017[no abstract]
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Optica Sensing Congress 2025 (AIS, Sensors, QSM)
A transponder-type laser interferometer is built to simulate tilt-to-length coupling in spaceborne gravitational wave interferometers. Intentional tilt of the detector and imaging system are used to suppress first-order and second-order TTL coupling.
Xiaoyang Lin +5 more
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A transponder-type laser interferometer is built to simulate tilt-to-length coupling in spaceborne gravitational wave interferometers. Intentional tilt of the detector and imaging system are used to suppress first-order and second-order TTL coupling.
Xiaoyang Lin +5 more
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Noise suppression of tilt-to-length coupling in space laser interferometer
Optics and Precision Engineering, 2021Lu-yu WANG, Yu-qiong LI, Rong CAI
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Classical and Quantum Gravity
Abstract Tilt-to-length (TTL) noise is one of the dominant noise sources in space-based gravitational wave (GW) detection. Methods such as the least squares estimator and the instrumental variables estimator can be employed to subtract TTL noise.
Hao-Kang Chen +2 more
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Abstract Tilt-to-length (TTL) noise is one of the dominant noise sources in space-based gravitational wave (GW) detection. Methods such as the least squares estimator and the instrumental variables estimator can be employed to subtract TTL noise.
Hao-Kang Chen +2 more
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Chinese Physics B
Abstract Tilt-to-length (TTL) coupling noise is a critical issue in space-based gravitational wave detection due to its complex dependence on multiple interacting factors, which complicates the identification of dominant parameters.
Fei 菲 Xie 谢 +4 more
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Abstract Tilt-to-length (TTL) coupling noise is a critical issue in space-based gravitational wave detection due to its complex dependence on multiple interacting factors, which complicates the identification of dominant parameters.
Fei 菲 Xie 谢 +4 more
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Classical and Quantum Gravity
Abstract Space gravitational wave telescopes are critical in achieving precise interstellar laser interferometry. The coupling coefficient is a key metric for evaluating the ultimate performance of a telescope. However, alignment errors during the assembly phase can degrade the wavefront quality of the telescope, intensify coupling noise,
Lanjun Huang +7 more
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Abstract Space gravitational wave telescopes are critical in achieving precise interstellar laser interferometry. The coupling coefficient is a key metric for evaluating the ultimate performance of a telescope. However, alignment errors during the assembly phase can degrade the wavefront quality of the telescope, intensify coupling noise,
Lanjun Huang +7 more
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Tilt-to-length coupling in LISA Pathfinder : Analytical modeling
Physical Review D, 2023Gudrun Wanner, Marie-Sophie Hartig
exaly