LISA Pathfinder: Understanding DWS noise performance for the LISA mission

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Wissel, L.: LISA Pathfinder: Understanding DWS noise performance for the LISA mission. In: Journal of Physics: Conference Series (JPCONF) 840 (2017), 012044. DOI: https://doi.org/10.1088/1742-6596/840/1/012044

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To cite the version in the repository, please use this identifier: https://doi.org/10.15488/16339

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Sum total of downloads: 28




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Abstract: 
ESA's L3 Laser Interferometer Space Antenna (LISA) mission contains a mechanism to compensate for out-of-plane angles between the received and emitted beams of the three satellites. Depending on the configuration of this Point-Ahead Angle Mechanism (PAAM) it is expected to contribute readout noise through Differential Wavefront Sensing (DWS). This was investigated with LISA Pathfinder (LPF) through a dedicated investigation. One of the two free-falling test masses was rotated via the on-board electrostatic actuators while the resulting angular noise in the differential interferometer between the two test masses was measured. For angles between -250 μrad to 250 μrad and corresponding contrast in the range of 59.4 % to 97.9 % an increased spectral density was found. The differential displacement noise remains almost unchanged for these misalignments.
License of this version: CC BY 3.0 Unported
Document Type: Article
Publishing status: publishedVersion
Issue Date: 2017
Appears in Collections:An-Institute

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pos. country downloads
total perc.
1 image of flag of Germany Germany 13 46.43%
2 image of flag of United States United States 4 14.29%
3 image of flag of Singapore Singapore 3 10.71%
4 image of flag of Taiwan Taiwan 2 7.14%
5 image of flag of China China 2 7.14%
6 image of flag of Netherlands Netherlands 1 3.57%
7 image of flag of Italy Italy 1 3.57%
8 image of flag of Indonesia Indonesia 1 3.57%
9 image of flag of Spain Spain 1 3.57%

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