NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Planetary radio astronomy receiverThe planetary radio astronomy (PRA) experiment on the Voyager spacecraft will measure the amplitude, spectrum, time variations, and polarization of radio emissions over a frequency range of 1.2 kHz to 40.5 MHz with the aid of the PRA receiver (PRAR) and two 10-m orthogonal monopoles. Sensitivity and dynamic range will allow observation of a wide range of Jovian emissions from near earth to encounter. This paper describes the system elements, including the preamp/attenuator/calibrator, the LF polarization discriminator, the four LF-IF amplifier stages, the HF polarization discriminator, the translation LO, the log-IF and detector, the frequency synthesizer, the data processor, control system, power supply, and antennas.
Document ID
19780026392
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lang, G. J.
(Martin Marietta Aerospace Denver, Colo., United States)
Peltzer, R. G.
(Colorado, University Boulder, Colo., United States)
Date Acquired
August 9, 2013
Publication Date
September 1, 1977
Publication Information
Publication: IEEE Transactions on Aerospace and Electronic Systems
Volume: AES-13
Subject Category
Astronomy
Accession Number
78A10301
Funding Number(s)
CONTRACT_GRANT: JPL-953592
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available