Chin. Phys. Lett.  2012, Vol. 29 Issue (6): 079501    DOI: 10.1088/0256-307X/29/7/079501
GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS |
Laser Interferometer Used for Satellite–Satellite Tracking: an On-Ground Methodological Demonstration
LI Yu-Qiong, LUO Zi-Ren, LIU He-Shan, DONG Yu-Hui, JIN Gang**
National Microgravity Laboratory (NML), Institute of Mechanics, Chinese Academy of Sciences, Beijing 100190
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LI Yu-Qiong, LUO Zi-Ren, LIU He-Shan et al  2012 Chin. Phys. Lett. 29 079501
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Abstract A Chinese satellite gravity mission called SAGM (Space Advanced Gravity Measurements) is now taken into consideration. To meet its designed requirement, the measurement precision of the laser ranging system used to measure the inter-satellite distance change has to be better than 100 nm/Hz1/2 within a broad bandwidth from 0.1 mHz to 1 Hz. An equal arm heterodyne Mach–Zehnder interferometer has been built on ground to demonstrate the measurement principle of a laser ranging system, which potentially can be used for both SAGM and future GW (gravitational wave) space antennas. Because of the equal arm length, the laser frequency noise has been significantly suppressed in the interferometer. Thus, the sensitivity better than 1 nm/Hz1/2 in a frequency range of 0.15 mHz–0.375 Hz has been achieved. The result shows that the proposed methodology has very promising feasibility to meet the requirements of SAGM and of GW space antennas as well.
Received: 15 March 2012      Published: 31 May 2012
PACS:  95.55.Br (Astrometric and interferometric instruments)  
  91.10.Pp (Geodetic techniques; gravimetric measurements and instruments)  
  42.60.By (Design of specific laser systems)  
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https://cpl.iphy.ac.cn/10.1088/0256-307X/29/7/079501       OR      https://cpl.iphy.ac.cn/Y2012/V29/I6/079501
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LI Yu-Qiong
LUO Zi-Ren
LIU He-Shan
DONG Yu-Hui
JIN Gang
[1] Danzmann K et al 1996 LISA Pre-Phase A Report, Max-Planck-Institut fur Quantenoptik Report No. MPQ 208 (Garching, Germany)
[2] Danzmann K et al 1996 Class. Quantum Grav. 13 A247
[3] Phinney S et al 2004 The Big Bang Observer: Direct Eetection of Gravitational Waves from the Birth of the Universe to the Present (NASA Mission Concept Study)
[4] Seto N, Kawamura S and Nakamura T 2001 Phys. Rev. Lett. 87 221103
[5] Bender P L 2004 Class Quantum Grav. 21 S1203
[6] Bender P L and Begelman M C 2005 Trends in Space Science and Cosmic Vision 2020 ESA SP-588 (Noordwijk: ESA Publications Division) p 33
[7] Bender P L, Hall J L, Ye J et al 2003 Space Sci. Rev. 108 377
[8] Sneeuw N, H Schaub 2005 Proceedings of IAG Symposia: Gravity, Geoid and Space Missions 129 12
[9] Shigeo N et al 2004 Meas. Sci. Technol. 15 2406
[10] Marina D et al 2009 J. Phys.: Conf. Ser. 154 012023
[11] Koop R and Rummel R 2007 The Future of Satellite Gravimetry, Final Report of the Future Gravity Mission Workshop
[12] Stebbins R T 2009 Class. Quantum Grav. 26 094014
[13] Gong X F et al 2011 Class. Quantum Grav. 28 094012
[14] Tapley B D, Bettadpur S, Watkins M et al 2004 Geophys. Res. Lett. 31 L09607
[15] Heinzel G et al 2006 Class. Quantum Grav. 23 S119
[16] Esteban J et al 2009 J. Phys.: Conf. Ser. 154 021025
[17] Heinzel G et al 2005 Class. Quantum Grav. 22 S149
[18] Armano M et al 2009 Class. Quantum Grav. 26 094001
[19] Bender P et al 2005 Conference on Laser and Electro-optics (Washington, DC: Optical Society of America) p 1754
[20] Yeh H et al 2011 Rev. Sci. Instrum. 82 044501
[21] Lu L Y et al 2009 Chin. J. Geophys. 52 2566 (in Chinese)
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