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Title: Plasma waves near Saturn: initial results from Voyager 1. Progress report

Technical Report ·
OSTI ID:5701374

The Voyager 1 plasma wave instrument detected many familiar types of plasma waves during the encounter with Saturn, including ion-acoustic waves and electron plasma oscillations upstream of the bow shock, an intense burst of electrostatic noise at the shock, and chorus, hiss, electrostatic (n + 1/2)fg waves and UHR emissions in the inner magnetosphere. A clock-like Saturn rotational control of low-frequency radio emissions was observed, and evidence was obtained of possible control by the moon Dione. Strong plasma wave emissions were detected at the Titan encounter indicating the presence of a turbulent sheath extending around Titan, and UHR measurements of the electron density show the existence of a dense plume of plasma being carried downstream of Titan by the interaction with the rapidly rotating magnetosphere of Saturn.

Research Organization:
Iowa Univ., Iowa City (USA). Dept. of Physics and Astronomy
OSTI ID:
5701374
Report Number(s):
AD-A-096321/5
Country of Publication:
United States
Language:
English