Logo image
Plasma Wave Observations with Cassini at Saturn
Conference presentation   Open access

Plasma Wave Observations with Cassini at Saturn

George B. Hospodarsky, J. D. Menietti, D. Pisa, W. S. Kurth, D. A. Gurnett, A. M. Persoon, J S Leisner and T. F. Averkamp
pp.277-289
Geophysical Monograph Book Series, Amer Geophysical Union
The 2014 Conference on Magnetosphere-Ionosphere Coupling (Yosemite National Park, 02/13/2014)
01/01/2017
DOI: 10.15142/T3G012
url
https://doi.org/10.15142/t3g012View
Open Access

Abstract

Since the Cassini spacecraft arrived at Saturn in 2004, the Radio and Plasma Wave Science (RPWS) -investigation has detected a variety of radio and plasma waves in the magnetosphere of Saturn, including whistler mode chorus and hiss, lightning-produced whistlers, high latitude auroral hiss, electrostatic electron cyclotron harmonic (ECH), upper hybrid resonance (UHR) and Langmuir wave emissions, Z-and O-mode narrowband emissions, and Saturn kilometric radiation (SKR). A number of these emissions often exhibit intensity modulations with periods ranging from about 10.6 to 10.8 hours. Plasma waves have also been detected in association with the Saturnian moons, including Enceladus and Rhea. We will review these observations and discuss the properties of the various waves.
Physical Sciences Astronomy & Astrophysics Geochemistry & Geophysics Science & Technology

Details

Metrics

5 Record Views
Logo image