Instrument Information |
|
IDENTIFIER | urn:nasa:pds:context:instrument:dsn.rss::1.0 |
NAME |
NASA DEEP SPACE NETWORK RADIO SCIENCE |
TYPE | |
DESCRIPTION |
Radio science and radio tracking instrumentation at the NASA Deep Space Network (DSN) utilize capabilities of the DSN in combination with telecommunications equipment on board spacecraft to make measurements that can be used to study gravity fields, relativistic effects, and the properties of plasmas, and planetary surfaces, atmospheres, ionospheres, and rings throughout the solar system. The DSN also sends commands to spacecraft and receives telemetry from them. This equipment may also be used for reception only, such as for radio astronomy observations of natural sources and for very long baseline interferometry. With few exceptions, this instrumentation is available for connection to any DSN antenna. Performance then depends on antenna size, wavelength, transmitter and low-noise amplifier selected, and local observing conditions. The instrumentation has evolved over time since the DSN was established in the 1960s. |
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NAIF INSTRUMENT IDENTIFIER | |
SERIAL NUMBER | |
REFERENCES |
Asmar, S. W., J. W. Armstrong, L. Iess, and P. Tortora, Spacecraft
Doppler Tracking: Noise Budget and Accuracy Achievable in Precision Radio
Science Observations, Radio Science, 40, RS2001, doi:10.1029/2004RS003101,
2005. Asmar, S. W., J. Lazio, D. H. Atkinson, D. J. Bell, J. S. Border, I. S. Grudinin, A. J. Mannucci, M. Paik, and R. A. Preston (2019). Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links, Radio Science, 54, 365-377. https://doi.org/10.1029/2018RS006663. Asmar, S.W., and N.A. Renzetti, The Deep Space Network as an Instrument for Radio Science Research, Jet Propulsion Laboratory Publication 80-93, Rev. 1, 15 April 1993. |