Precision of Spacecraft Doppler Tracking at Low Signal‐To‐Noise Ratios

Author:

Buccino D. R.1ORCID,Oudrhiri K.1,Parisi M.1ORCID,Park R. S.1ORCID,Mazarico E.2ORCID,Tortora P.34ORCID,Withers P.5ORCID,Genova A.6ORCID,Zannoni M.34ORCID

Affiliation:

1. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

2. Goddard Space Flight Center National Aeronautics and Space Administration Greenbelt MD USA

3. Department of Industrial Engineering Alma Mater Studiorum ‐ Università di Bologna Bologna Italy

4. Centro Interdipartimentale di Ricerca Industriale Aerospaziale Alma Mater Studiorum ‐ Università di Bologna Bologna Italy

5. Boston University Boston MA USA

6. Dipartimento di Ingegneria Aerospaziale e Astronautica Università di Roma “La Sapienza” Rome Italy

Abstract

AbstractThe signal‐to‐noise ratio received at Earth is typically larger than 10 dB‐Hz for radio tracking of a spacecraft in deep space, allowing a phase‐locked loop to execute reliable carrier tracking. Recently, missions have been proposed to utilize low‐gain antennas for Doppler tracking where the signal‐to‐noise ratio may be at the single‐digit (dB‐Hz) level. In this work, we discuss spacecraft Doppler tracking at these low signal‐to‐noise ratios through an analysis of thermal noise on the radio link, results from ground testing with the Deep Space Network, and demonstrations with an active spacecraft. We show that by utilizing an open‐loop receiver to capture the carrier signal and by applying post‐processing techniques, radio data with the signal‐to‐noise ratio as low as 4 dB‐Hz can be used to derive Doppler data with precision sufficient for tracking a spacecraft in deep space.

Funder

National Aeronautics and Space Administration

Agenzia Spaziale Italiana

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

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