Radio and Plasma Wave Observations at Saturn from Cassini's Approach and First Orbit

Author:

Gurnett D. A.12345,Kurth W. S.12345,Hospodarsky G. B.12345,Persoon A. M.12345,Averkamp T. F.12345,Cecconi B.12345,Lecacheux A.12345,Zarka P.12345,Canu P.12345,Cornilleau-Wehrlin N.12345,Galopeau P.12345,Roux A.12345,Harvey C.12345,Louarn P.12345,Bostrom R.12345,Gustafsson G.12345,Wahlund J.-E.12345,Desch M. D.12345,Farrell W. M.12345,Kaiser M. L.12345,Goetz K.12345,Kellogg P. J.12345,Fischer G.12345,Ladreiter H.-P.12345,Rucker H.12345,Alleyne H.12345,Pedersen A.12345

Affiliation:

1. Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA.

2. Observatoire de Paris, 92195 Meudon, France.

3. Centre d'Etude des Environments Terrestre et Planétaires (CETP)–L'Institut Pierre-Simon La Place, 78140 Velizy, France.

4. Centre d'Etude Spatiale des Rayonnements–CNRS, 31028 Toulouse, France.

5. Swedish Institute of Space Physics, SE-751 21 Uppsala, Sweden.

Abstract

We report data from the Cassini radio and plasma wave instrument during the approach and first orbit at Saturn. During the approach, radio emissions from Saturn showed that the radio rotation period is now 10 hours 45 minutes 45 ± 36 seconds, about 6 minutes longer than measured by Voyager in 1980 to 1981. In addition, many intense impulsive radio signals were detected from Saturn lightning during the approach and first orbit. Some of these have been linked to storm systems observed by the Cassini imaging instrument. Within the magnetosphere, whistler-mode auroral hiss emissions were observed near the rings, suggesting that a strong electrodynamic interaction is occurring in or near the rings.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference32 articles.

1. The Cassini Radio and Plasma Wave Investigation

2. Voyager Detection of Nonthermal Radio Emission from Saturn

3. M. L. Kaiseret al., in Saturn, T. Gehrels, M. Shapley-Matthews, Eds. (Arizona Press, Tucson, 1984), pp. 378–415.

4. M. E. Davies et al., Celest. Mech. Dyn. Astron.63, 127 (1996).

5. A. Lecacheux, P. H. M. Galopeau, M. Aubier, in Planetary Radio Emissions IV, H. Rucker, S. Bauer, A. Lecacheux, Eds. (Austrian Academy of Science, Vienna, 1997), pp. 313–325.

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