Spacecraft and interplanetary contributions to the magnetic environment on-board LISA Pathfinder

Author:

Armano M1,Audley H2,Baird J3,Binetruy P3,Born M2,Bortoluzzi D4,Castelli E5,Cavalleri A6,Cesarini A7,Cruise A M8,Danzmann K2,de Deus Silva M9,Diepholz I2,Dixon G8,Dolesi R5,Ferraioli L9,Ferroni V5,Fitzsimons E D10,Freschi M11,Gesa L12,Gibert F5,Giardini D9,Giusteri R5,Grimani C7,Grzymisch J1,Harrison I13,Hartig M-S2,Heinzel G2,Hewitson M2,Hollington D14,Hoyland D8,Hueller M5,Inchauspé H315,Jennrich O1,Jetzer P16,Karnesis N3,Kaune B2,Korsakova N17,Killow C J17,Lobo J A12,Liu L5,López-Zaragoza J P12ORCID,Maarschalkerweerd R13,Mance D9,Martín V12,Martin-Polo L11,Martino J3,Martin-Porqueras F11,Mateos I12,McNamara P W1,Mendes J13,Mendes L11,Meshksar N9,Nofrarias M12ORCID,Paczkowski S2,Perreur-Lloyd M17,Petiteau A3,Pivato P5,Plagnol E3,Ramos-Castro J18,Reiche J2,Rivas F12,Robertson D I17,Roma-Dollase D12,Russano G5,Slutsky J,Sopuerta C F12,Sumner T14,Telloni D19,Texier D11,Thorpe J I,Trenkel C20,Vetrugno D5,Vitale S5,Wanner G2,Ward H17,Wass P J14,Wealthy D20,Weber W J5,Wissel L2,Wittchen A2,Zweifel P9

Affiliation:

1. European Space Technology Centre, European Space Agency, Keplerlaan 1, NL-2200 AG Noordwijk, the Netherlands

2. Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, D-30167 Hannover, Germany

3. APC, Paris Diderot University, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne Paris Cité 75013, France

4. Department of Industrial Engineering, University of Trento and Trento Institute for Fundamental Physics and Applications/INFN, Via Sommarive 9, I-38123 Trento, Italy

5. Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Applications/INFN, I-38123 Povo, Trento, Italy

6. Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy

7. DISPEA, Università di Urbino ‘Carlo Bo’, Via S. Chiara 27, I-61029 Urbino/INFN, Italy

8. The School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, UK

9. European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, E-28692 Madrid, Spain

10. Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland

11. The UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK

12. Institut de Ciències de l’Espai (CSIC-IEEC), Campus UAB, Carrer de Can Magrans s/n, E-08193 Cerdanyola del Vallès, Spain

13. European Space Operations Centre, European Space Agency, D-64293 Darmstadt, Germany

14. High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2BW, UK

15. Department of Mechanical and Aerospace Engineering, University of Florida, MAE-A, P.O. Box 116250, Gainesville, FL 32611, USA

16. Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland

17. SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK

18. Department d’Enginyeria Electrònica, Universitat Politècnica de Catalunya, E-08034 Barcelona, Spain

19. National Institute for Astrophysics, Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese (TO), Italy

20. Airbus Defence and Space, Gunnels Wood Road, Stevenage, Hertfordshire SG1 2AS, UK

Abstract

ABSTRACT LISA Pathfinder (LPF) has been a space-based mission designed to test new technologies that will be required for a gravitational wave observatory in space. Magnetically driven forces play a key role in the instrument sensitivity in the low-frequency regime (mHz and below), the measurement band of interest for a space-based observatory. The magnetic field can couple to the magnetic susceptibility and remanent magnetic moment from the test masses and disturb them from their geodesic movement. LPF carried on-board a dedicated magnetic measurement subsystem with noise levels of 10 $\rm nT \ Hz^{-1/2}$ from 1 Hz down to 1 mHz. In this paper we report on the magnetic measurements throughout LPF operations. We characterize the magnetic environment within the spacecraft, study the time evolution of the magnetic field and its stability down to 20 μHz, where we measure values around 200 $\rm nT \ Hz^{-1/2}$, and identify two different frequency regimes, one related to the interplanetary magnetic field and the other to the magnetic field originating inside the spacecraft. Finally, we characterize the non-stationary component of the fluctuations of the magnetic field below the mHz and relate them to the dynamics of the solar wind.

Funder

CNES

UnivEarthS Labex

DLR

Federal Ministry for Economic Affairs and Energy

Agenzia Spaziale Italiana

Instituto Nazionale di Fisica Nucleare

MICINN

MINECO

Fundación General CSIC

ESA

Swiss National Science Foundation

United Kingdom Space Agency

University of Glasgow

University of Birmingham

Scottish Universities Physics Alliance

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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