Sensor noise in LISA Pathfinder: An extensive in-flight review of the angular and longitudinal interferometric measurement system

被引：34

作者：

Armano, M. ^{[1
]}

Audley, H. ^{[2
,3
]}

Baird, J. ^{[4
]}

Binetruy, P. ^{[4
]}

Born, M. ^{[2
,3
]}

Bortoluzzi, D. ^{[5
,6
]}

Brandt, N. ^{[7
]}

Castelli, E. ^{[6
,8
]}

Cavalleri, A. ^{[9
]}

Cesarini, A. ^{[10
]}

Cruise, A. M. ^{[11
]}

Danzmann, K. ^{[2
,3
]}

Silva, M. de Deus ^{[12
]}

Diepholz, I. ^{[2
,3
]}

Dixon, G. ^{[11
]}

Dolesi, R. ^{[6
,8
]}

Ferraioli, L. ^{[13
]}

Ferroni, V. ^{[6
,8
]}

Fitzsimons, E. D. ^{[14
]}

Flatscher, R. ^{[7
]}

Freschi, M. ^{[12
]}

Garcia, A. ^{[15
]}

Gerndt, R. ^{[7
]}

Gesa, L. ^{[16
,17
]}

Giardini, D. ^{[13
]}

Gibert, F. ^{[6
,8
,18
]}

Giusteri, R. ^{[2
,3
]}

Grimani, C. ^{[10
]}

Grzymisch, J. ^{[1
]}

Guzman, F. ^{[19
]}

Harrison, I. ^{[20
]}

Hartig, M-S ^{[2
,3
]}

Hechenblaikner, G. ^{[7
]}

Heinzel, G. ^{[2
,3
]}

Hewitson, M. ^{[2
,3
]}

Hollington, D. ^{[21
]}

Hoyland, D. ^{[11
]}

Hueller, M. ^{[6
,8
]}

Inchauspe, H. ^{[4
,22
]}

Jennrich, O. ^{[1
]}

Jetzer, P. ^{[23
]}

Johann, U. ^{[7
]}

Johlander, B. ^{[1
]}

Karnesis, N. ^{[4
]}

Kaune, B. ^{[2
,3
]}

Killow, C. J. ^{[24
]}

Korsakova, N. ^{[25
]}

Lobo, J. A. ^{[16
,17
]}

Lopez-Zaragoza, J. P. ^{[16
,17
]}

Maarschalkerweerd, R. ^{[20
]}

机构：

[1] European Space Agcy, European Space Technol Ctr, Keplerlaan 1, NL-2200 AG Noordwijk, Netherlands

[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[3] Leibniz Univ Hannover, D-30167 Hannover, Germany

[4] Univ Paris, APC, CNRS, Astroparticule & Cosmol, F-75006 Paris, France

[5] Univ Trento, Dept Ind Engn, Via Sommar 9, I-38123 Trento, Italy

[6] Ist Nazl Fis Nucl, Trento Inst Fundamental Phys & Applicat, I-38123 Povo, Trento, Italy

[7] Airbus Def & Space, Claude Dornier Str, D-88090 Immenstaad, Germany

[8] Univ Trento, Dipartimento Fis, I-38123 Povo, Trento, Italy

[9] CNR Fdn Bruno Kessler, Ist Foton & Nanotecnol, I-38123 Povo, Trento, Italy

[10] Univ Urbino Carlo Bo, DISPEA, Via S Chiara 27, I-61029 Urbino, Italy

[11] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[12] European Space Agcy, European Space Astron Ctr, Madrid 28692, Spain

[13] Swiss Fed Inst Technol, Inst Geophys, Sonneggstr 5, CH-8092 Zurich, Switzerland

[14] Royal Observ, UK Astron Technol Ctr, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[15] City Univ Appl Sci, Flughafenallee 10, D-28199 Bremen, Germany

[16] CSIC, ICE, Campus UAB,Carrer Can Magrans S-N, Cerdanyola Del Valles 08193, Spain

[17] IEEC, C Gran Capita 2-4, Barcelona 08034, Spain

[18] isardSAT SL, Marie Curie 8-14, Barcelona 08042, Catalonia, Spain

[19] Texas A&M Univ, 701 HR Bright Bldg, College Stn, TX 77843 USA

[20] European Space Agcy, European Space Operat Ctr, D-64293 Darmstadt, Germany

[21] Imperial Coll London, Phys Dept, Blackett Lab, High Energy Phys Grp, Prince Consort Rd, London SW7 2BW, England

[22] Univ Florida, Dept Mech & Aerosp Engn, MAE A, POB 116250, Gainesville, FL 32611 USA

[23] Univ Zurich, Phys Inst, Winterthurerstr 190, CH-8057 Zurich, Switzerland

[24] Univ Glasgow, Inst Gravitat Res, Sch Phys & Astron, SUPA, Glasgow G12 8QQ, Lanark, Scotland

[25] Observ Cote Azur, Blvd Observ CS 34229-F, F-06304 Nice, France

[26] OHB Syst AG, Univ Allee 27-29, D-28359 Bremen, Germany

[27] Univ Politecn Cataluna, Dept Engn Elect, Barcelona 08034, Spain

[28] Univ Loyola Andalucia, Dept Quantitat Methods, Ave Univ S-N, Dos Hermanas 41704, Sevilla, Spain

[29] Univ Florida, Dept Phys, 2001 Museum Rd, Gainesville, FL 32611 USA

[30] NASA, Gravitat Astrophys Lab, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

来源：

PHYSICAL REVIEW D | 2022年 / 106卷 / 08期

基金：

瑞士国家科学基金会; 美国国家航空航天局;

关键词：

LTP INTERFEROMETER; AUTOMATIC ALIGNMENT; OPTICAL WINDOW; DRAG-FREE; CONSTRUCTION; DIAGNOSTICS; PHASE;

D O I：

10.1103/PhysRevD.106.082001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In a previous article [1], we have reported on the first subpicometer interferometer flown in space as part of ESA's LISA Pathfinder mission, and have shown the residual sensor noise to be on the level of 32.0 thorn 2.4 -1.7 fm/ . This review provides a deeper and more complete overview of the full system and its ffiffiffiffiffiHz interferometric mission performance under varying operational conditions, allowing a much more detailed view on the noise model. We also include the optical measurements of rotations through differential wave ffiffiffiffiffifront sensing (DWS), which reached a sensitivity of as good as 100 prad/ Hz. We present more evidence for the long-term stability of the interferometric performance and components. This proves a solid foundation for future interferometry in space such as the LISA mission.

引用

页数：34

共 73 条

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