Design of dedicated tilt-to-length calibration maneuvers for LISA

Tilts of certain elements within a laser interferometer can undesirably couple into measurements as a form of noise, known as tilt-to-length (TTL) coupling. This TTL coupling is anticipated to be one of the primary noise sources in the Laser Interferometer Space Antenna mission, after time delay interferometry is applied. Despite the careful interferometer design and calibration on the ground, TTL is likely to require in-flight mitigation through postprocessing subtraction to achieve the necessary sensitivity. Past research has demonstrated TTL subtraction in simulations through the estimation of 24 linear coupling coefficients using a noise minimization approach. This paper investigates an approach based on performing rotation maneuvers for estimating coupling coefficients with low uncertainties. In this study, we evaluate the feasibility and optimal configurations of such maneuvers to identify the most efficient solutions. We assess the efficacy of TTL calibration maneuvers by modulating either the spacecraft attitude or the moving optical subassembly yaw angle. We found that sinusoidal signals with amplitudes of around 30 nrad and frequencies near 43 mHz are practical and nearly optimal choices for such modulations. Employing different frequencies generates uncorrelated signals, allowing for multiple maneuvers to be executed simultaneously. Our simulations enable us to estimate the TTL coefficients with precision below <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mn>15</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi mathvariant="normal">μ</a:mi><a:mi mathvariant="normal">m</a:mi><a:mo>/</a:mo><a:mi>rad</a:mi></a:mrow></a:math> (<e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mn>1</e:mn><e:mtext>−</e:mtext><e:mi>σ</e:mi></e:math>, in free space) after a total maneuver time of 20 min. The results are compared to the estimation uncertainties that can be achieved without using maneuvers.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-05-23
DOI
https://doi.org/10.1103/ndwh-vr2y
Citations
2
Primary Topic
Particle accelerators and beam dynamics
Type
article
Field-Weighted Citation Impact
9.99
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article

Design of dedicated tilt-to-length calibration maneuvers for LISA

Gerhard Heinzel, S. Paczkowski, Gudrun Wanner, Marie-Sophie Hartig et al.
2 citations
Physical review. D/Physical review. D.
Particle accelerators and beam dynamics
9.99
article

Design of dedicated tilt-to-length calibration maneuvers for LISA

Gerhard Heinzel, S. Paczkowski, Gudrun Wanner, Marie-Sophie Hartig, M. Hewitson, Karl J. Friston
article en
2 citations

Abstract

Tilts of certain elements within a laser interferometer can undesirably couple into measurements as a form of noise, known as tilt-to-length (TTL) coupling. This TTL coupling is anticipated to be one of the primary noise sources in the Laser Interferometer Space Antenna mission, after time delay interferometry is applied. Despite the careful interferometer design and calibration on the ground, TTL is likely to require in-flight mitigation through postprocessing subtraction to achieve the necessary sensitivity. Past research has demonstrated TTL subtraction in simulations through the estimation of 24 linear coupling coefficients using a noise minimization approach. This paper investigates an approach based on performing rotation maneuvers for estimating coupling coefficients with low uncertainties. In this study, we evaluate the feasibility and optimal configurations of such maneuvers to identify the most efficient solutions. We assess the efficacy of TTL calibration maneuvers by modulating either the spacecraft attitude or the moving optical subassembly yaw angle. We found that sinusoidal signals with amplitudes of around 30 nrad and frequencies near 43 mHz are practical and nearly optimal choices for such modulations. Employing different frequencies generates uncorrelated signals, allowing for multiple maneuvers to be executed simultaneously. Our simulations enable us to estimate the TTL coefficients with precision below <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mn>15</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi mathvariant="normal">μ</a:mi><a:mi mathvariant="normal">m</a:mi><a:mo>/</a:mo><a:mi>rad</a:mi></a:mrow></a:math> (<e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mn>1</e:mn><e:mtext>−</e:mtext><e:mi>σ</e:mi></e:math>, in free space) after a total maneuver time of 20 min. The results are compared to the estimation uncertainties that can be achieved without using maneuvers.

Physical review. D/Physical review. D.Vol. 112(2)
Leibniz University Hannover (DE), Max Planck Institute for Gravitational Physics (DE)
Affordable and clean energy
Openalex Percentile: Top 3%
Particle accelerators and beam dynamics
9.99
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