Planetary Radio Interferometry and Doppler Experiment (PRIDE) technique: A test case of the Mars Express Phobos fly-by

被引：27

作者：

Duev, D. A. ^{[1
,2
,3
]}

Pogrebenko, S. V. ^{[2
]}

Cimo, G. ^{[2
,4
]}

Molera Calves, G. ^{[2
,5
]}

Bahamon, T. M. Bocanegra ^{[2
,6
,7
]}

Gurvits, L. I. ^{[2
,6
]}

Kettenis, M. M. ^{[2
]}

Kania, J. ^{[2
,8
]}

Tudose, V. ^{[9
]}

Rosenblatt, P. ^{[10
]}

Marty, J. -C. ^{[11
]}

Lainey, V. ^{[12
]}

de Vicente, P. ^{[13
]}

Quick, J. ^{[14
]}

Nickola, M. ^{[14
]}

Neidhardt, A. ^{[15
]}

Kronschnabl, G. ^{[15
]}

Ploetz, C. ^{[15
]}

Haas, R. ^{[16
]}

Lindqvist, M. ^{[16
]}

Orlati, A. ^{[17
]}

Ipatov, A. V. ^{[18
]}

Kharinov, M. A. ^{[18
]}

Mikhailov, A. G. ^{[18
]}

Lovell, J. E. J. ^{[19
]}

McCallum, J. N. ^{[19
]}

Stevens, J. ^{[20
]}

Gulyaev, S. A. ^{[21
]}

Natush, T. ^{[21
]}

Weston, S. ^{[21
]}

Wang, W. H. ^{[7
]}

Xia, B. ^{[7
]}

Yang, W. J. ^{[22
]}

Hao, L. -F. ^{[23
]}

Kallunki, J. ^{[24
]}

Witasse, O. ^{[25
]}

机构：

[1] CALTECH, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[2] Joint Inst VLBI ERIC, POB 2, NL-7990 AA Dwingeloo, Netherlands

[3] Lomonosov Moscow State Univ, Sternberg Astron Inst, Univ Av 13, Moscow 119991, Russia

[4] Netherlands Inst Radio Astron, ASTRON, Postbus 2, NL-7990 AA Dwingeloo, Netherlands

[5] Aalto Univ, Sch Elect Engn, Dept Radio Sci & Engn, Espoo 02150, Finland

[6] Delft Univ Technol, Dept Astrodynam & Space Missions, NL-2629 HS Delft, Netherlands

[7] Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China

[8] Carnegie Mellon Univ, 5000 Forbes Ave, Pittsburgh, PA 15213 USA

[9] Inst Space Sci, Atomistilor 409,POB MG-23, Bucharest 077125, Romania

[10] Royal Observ Belgium, Ringlaan 3, B-1180 Brussels, Belgium

[11] CNES GRGS, OMP 14 Ave Edouard Belin, F-31400 Toulouse, France

[12] UPMC Lille 1, CNRS, PSL Res Univ, UMR CNRS 8028,IMCCE,Observ Paris, 77 Av Denfert Rochereau, F-75014 Paris, France

[13] Observ Yebes IGN, Apartado 148, Guadalajara 19180, Spain

[14] Hartebeesthoek Radio Astron Observ, ZA-1740 Krugersdorp, South Africa

[15] Geodet Observ Wettzell, Fed Agcy Cartog & Geodesy, D-60598 Frankfurt, Germany

[16] Chalmers Univ Technol, Dept Earth & Space Sci, Onsala Space Observ, S-43992 Onsala, Sweden

[17] Radio Observ Medicina, Natl Inst Astrophys, Radio Astron Inst, I-75500 Medicina, Italy

[18] Russian Acad Sci, Inst Appl Astron, Kutuzova Embankment 10, St Petersburg 191187, Russia

[19] Univ Tasmania, Sch Phys Sci, Private Bag 37, Hobart, Tas 7001, Australia

[20] Australia Telescope Natl Facil, CSIRO Astron & Space Sci, Narrabri, NSW 2390, Australia

[21] Auckland Univ Technol, Inst Radio Astron & Space Res, Private Bag 92006, Auckland 1142, New Zealand

[22] Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China

[23] Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China

[24] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland

[25] European Space Agcy ESA ESTEC Sci Support Off, NL-2200 AG Noordwijk, Netherlands

来源：

ASTRONOMY & ASTROPHYSICS | 2016年 / 593卷

关键词：

techniques: interferometric; techniques: miscellaneous; methods: data analysis; astrometry; VLBI;

D O I：

10.1051/0004-6361/201628869

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Context. The closest ever fly-by of the Martian moon Phobos, performed by the European Space Agency's Mars Express spacecraft, gives a unique opportunity to sharpen and test the Planetary Radio Interferometry and Doppler Experiments (PRIDE) technique in the interest of studying planet-satellite systems. Aims. The aim of this work is to demonstrate a technique of providing high precision positional and Doppler measurements of planetary spacecraft using the Mars Express spacecraft. The technique will be used in the framework of Planetary Radio Interferometry and Doppler Experiments in various planetary missions, in particular in fly-by mode. Methods. We advanced a novel approach to spacecraft data processing using the techniques of Doppler and phase-referenced very long baseline interferometry spacecraft tracking. Results. We achieved, on average, mHz precision (30 mu m/s at a 10 s integration time) for radial three-way Doppler estimates and sub-nanoradian precision for lateral position measurements, which in a linear measure (at a distance of 1.4 AU) corresponds to similar to 50 m.

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