Plasma waves near Saturn: initial results from Voyager 1. Progress report
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
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Related Subjects
GENERAL PHYSICS
SATURN PLANET
PLASMA WAVES
ELECTRON DENSITY
ION ACOUSTIC WAVES
PLANETARY MAGNETOSPHERES
RADIOWAVE RADIATION
SHOCK WAVES
SPACE VEHICLES
VOYAGER SPACE PROBES
ATMOSPHERES
ELECTROMAGNETIC RADIATION
ION WAVES
PLANETARY ATMOSPHERES
PLANETS
RADIATIONS
VEHICLES
640107* - Astrophysics & Cosmology- Planetary Phenomena