Density and Temperature of the Electron Core in the Inner Magnetosphere of Saturn from Cassini/RPWS Antennas (abstract)

M. Moncuquet; M. E. Gkini

doi:doi:10.1553/PRE7s133

H.O. Rucker - W.S. Kurth - P. Louarn - G. Fischer (Eds.)

Planetary Radio Emissions VII

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010

Helmut Rucker
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

William Kurth
Department of Physics and Astronomy, University of Iowa, Iowa City, USA

Philippe Louarn
Centre d'Etude Spatiale de Rayonnements, CNRS/Universitè Paul-Sabatier Toulouse III, Toulouse, France

Georg Fischer
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

ISBN 978-3-7001-7125-6 Print Edition
ISBN 978-3-7001-7246-8 Online Edition

doi: https://doi.org/10.1553/PRE7

2011 578 Seiten, 23x15cm, broschiert
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The 7th International Workshop on "Planetary, Solar and Heliospheric Radio Emissions" is the continuation of an established tradition: This PRE VII conference followed previous successful international workshops held at Graz, Austria, in 1984, 1987, 1991, 1996, 2001, and 2005. This 7th workshop in September 2010 offered again the unique opportunity to discuss the observations from Cassini at Saturn and to investigate the measurements by other spacecraft and from the ground of the Jovian, terrestrial and solar radio emissions, also including studies on radiation from exoplanetary sources.

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Density and Temperature of the Electron Core in the Inner Magnetosphere of Saturn from Cassini/RPWS Antennas (abstract)

M. Moncuquet,

M. E. Gkini

Planetary Radio Emissions VII, pp. 133-134, 2011/12/28

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010

doi: 10.1553/PRE7s133

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doi:10.1553/PRE7s133

Abstract

We study the large scale structures of the electron core in the inner magnetosphere of Saturn (from the G-ring to Rhea orbit - i.e. 2.8 to 9 Rs). This study is deduced from the power spectra measurements acquired with the Cassini/RPWS electric dipole around the local plasma frequency (quasi-thermal noise spectroscopy), from July 2004 (SOI) to February 2010. We have especially investigated the radial diffusion and latitudinal confinement of the plasma torus towards Enceladus and Dione. We also discuss the longitudinal variations of the electron parameters using the recent SLS3 system. We will finally touch about the dust detection by using the RF power spectra measured on the monopole antenna and the possible effect of the dust on the observed electron parameters.

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Published Online: 2011/12/28 13:41:56

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H.O. Rucker - W.S. Kurth - P. Louarn - G. Fischer (Eds.)

Planetary Radio Emissions VII

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010

Density and Temperature of the Electron Core in the Inner Magnetosphere of Saturn from Cassini/RPWS Antennas (abstract)

€ 79,–

Abstract