Details
Original language | English |
---|---|
Article number | 29 |
Pages (from-to) | 164-173 |
Number of pages | 10 |
Journal | Proceedings of SPIE - The International Society for Optical Engineering |
Volume | 5500 |
Publication status | Published - 29 Sept 2004 |
Externally published | Yes |
Event | Gravitational Wave and Particle Astrophysics Detectors - Glasgow, United Kingdom (UK) Duration: 23 Jun 2004 → 24 Jun 2004 |
Abstract
The LISA Technology Package (LTP) aboard of LISA pathfinder mission is dedicated to demonstrate and verify key technologies for LISA, in particular drag free control, ultra-precise laser interferometry and gravitational sensors. Two inertial sensors, the optical interferometry in between combined with the dimensional stable Glass ceramic Zerodur structure are setting up the LTP. The validation of drag free operation of the spacecraft is planned by measuring laser interferometrically the relative displacement and tilt between two test masses (and the optical bench) with a noise levels of 10pm/√Hz and 10nrad/√Hz between 30 mHz and 30mHz. This performance and additionally overall environmental tests was currently verified on EM level. The OB structure is able to support two inertial sensors (≈17 kg each) and to withstand 25 g design loads as well as 0...40°C temperature range. Optical functionality was verified successfully after environmental tests. The engineering model development and manufacturing of the optical bench and interferometry hardware and their verification tests will be presented.
Keywords
- Gravitational wave, Inertial sensor, LISA pathfinder, Optical bench, Optical interferometry, Zerodur structure
ASJC Scopus subject areas
- Materials Science(all)
- Electronic, Optical and Magnetic Materials
- Physics and Astronomy(all)
- Condensed Matter Physics
- Computer Science(all)
- Computer Science Applications
- Mathematics(all)
- Applied Mathematics
- Engineering(all)
- Electrical and Electronic Engineering
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In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 5500, 29, 29.09.2004, p. 164-173.
Research output: Contribution to journal › Conference article › Research › peer review
}
TY - JOUR
T1 - LISA pathfinder optical interferometry
AU - Braxmaier, C.
AU - Heinzel, G.
AU - Middleton, K.
AU - Caldwell, M.
AU - Konrad, W.
AU - Stockburger, H.
AU - Lucarelli, S.
AU - Te Plate, M.
AU - Wand, V.
AU - Garcia, A. C.
AU - Draaisma, F.
AU - Pijnenburg, J.
AU - Robertson, D.
AU - Killow, C.
AU - Ward, H.
AU - Danzmann, K.
AU - Johann, U.
PY - 2004/9/29
Y1 - 2004/9/29
N2 - The LISA Technology Package (LTP) aboard of LISA pathfinder mission is dedicated to demonstrate and verify key technologies for LISA, in particular drag free control, ultra-precise laser interferometry and gravitational sensors. Two inertial sensors, the optical interferometry in between combined with the dimensional stable Glass ceramic Zerodur structure are setting up the LTP. The validation of drag free operation of the spacecraft is planned by measuring laser interferometrically the relative displacement and tilt between two test masses (and the optical bench) with a noise levels of 10pm/√Hz and 10nrad/√Hz between 30 mHz and 30mHz. This performance and additionally overall environmental tests was currently verified on EM level. The OB structure is able to support two inertial sensors (≈17 kg each) and to withstand 25 g design loads as well as 0...40°C temperature range. Optical functionality was verified successfully after environmental tests. The engineering model development and manufacturing of the optical bench and interferometry hardware and their verification tests will be presented.
AB - The LISA Technology Package (LTP) aboard of LISA pathfinder mission is dedicated to demonstrate and verify key technologies for LISA, in particular drag free control, ultra-precise laser interferometry and gravitational sensors. Two inertial sensors, the optical interferometry in between combined with the dimensional stable Glass ceramic Zerodur structure are setting up the LTP. The validation of drag free operation of the spacecraft is planned by measuring laser interferometrically the relative displacement and tilt between two test masses (and the optical bench) with a noise levels of 10pm/√Hz and 10nrad/√Hz between 30 mHz and 30mHz. This performance and additionally overall environmental tests was currently verified on EM level. The OB structure is able to support two inertial sensors (≈17 kg each) and to withstand 25 g design loads as well as 0...40°C temperature range. Optical functionality was verified successfully after environmental tests. The engineering model development and manufacturing of the optical bench and interferometry hardware and their verification tests will be presented.
KW - Gravitational wave
KW - Inertial sensor
KW - LISA pathfinder
KW - Optical bench
KW - Optical interferometry
KW - Zerodur structure
UR - http://www.scopus.com/inward/record.url?scp=19944404739&partnerID=8YFLogxK
U2 - 10.1117/12.555266
DO - 10.1117/12.555266
M3 - Conference article
AN - SCOPUS:19944404739
VL - 5500
SP - 164
EP - 173
JO - Proceedings of SPIE - The International Society for Optical Engineering
JF - Proceedings of SPIE - The International Society for Optical Engineering
SN - 0277-786X
M1 - 29
T2 - Gravitational Wave and Particle Astrophysics Detectors
Y2 - 23 June 2004 through 24 June 2004
ER -