title: Planetary radio astronomy observations from voyager 1 near saturn.
abstract: The Voyager 1 planetary radio astronomy experiment detected two distinct kinds of radio emissions from Saturn. The first, Saturn kilometric radiation, is strongly polarized, bursty, tightly correlated with Saturn's rotation, and exhibits complex dynamic spectral features somewhat reminiscent of those in Jupiter's radio emission. It appears in radio frequencies below about 1.2 megahertz. The second kind of radio emission, Saturn electrostatic discharge, is unpolarized, extremely impulsive, loosely correlated with Saturn's rotation, and very broadband, appearing throughout the observing range of the experiment (20.4 kilohertz to 40.2 megahertz). Its sources appear to lie in the planetary rings.
authors.forename: J W
authors.initials: JW
authors.lastname: Warwick
authors.forename: J B
authors.initials: JB
authors.lastname: Pearce
authors.forename: D R
authors.initials: DR
authors.lastname: Evans
authors.forename: T D
authors.initials: TD
authors.lastname: Carr
authors.forename: J J
authors.initials: JJ
authors.lastname: Schauble
authors.forename: J K
authors.initials: JK
authors.lastname: Alexander
authors.forename: M L
authors.initials: ML
authors.lastname: Kaiser
authors.forename: M D
authors.initials: MD
authors.lastname: Desch
authors.forename: M
authors.initials: M
authors.lastname: Pedersen
authors.forename: A
authors.initials: A
authors.lastname: Lecacheux
authors.forename: G
authors.initials: G
authors.lastname: Daigne
authors.forename: A
authors.initials: A
authors.lastname: Boischot
authors.forename: C H
authors.initials: CH
authors.lastname: Barrow