Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.
Submitted on September 17, 2004
Accepted on November 29, 2004
Radio and Plasma Wave Observations at Saturn from Cassini's Approach and First Orbit
D. A. Gurnett 1*, W. S. Kurth 1, G. B. Hospodarsky 1, A. M. Persoon 1, T. F. Averkamp 1, B. Cecconi 1, A. Lecacheux 2, P. Zarka 2, P Canu 3, N. Cornilleau-Wehrlin 3, P. Galopeau 3, A. Roux 3, C. Harvey 4, P. Louarn 4, R. Bostrom 5, G. Gustafsson 5, J.-E. Wahlund 5, M. D. Desch 6, W. M. Farrell 6, M. L. Kaiser 6, K. Goetz 7, P. J. Kellogg 7, G. Fischer 8, H.-P. Ladreiter 8, H. Rucker 8, H. Alleyne 9, A. Pedersen 10
1 Univ. of Iowa, Dept. of Physics and Astronomy, Iowa City, IA 52242, USA. 2 Observatoire de Paris, 92195 Meudon, France. 3 CETP-IPSL, 78140 Velizy, France. 4 CESR-CNRS, 31028, Toulouse, France. 5 Swedish Inst. of Space Physics, SE-751 21 Uppsala, Sweden. 6 NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA. 7 Univ. of Minnesota, Dept. of Physics and Astronomy, Minneapolis, MN 55455, USA. 8 Austrian Academy of Sciences, Space Research Institute, A-8042 Graz, Austria. 9 Univ. of Sheffield, Dept. of Automatic Control & Systems Eng., Sheffield S1 4DU, UK. 10 Univ. of Oslo, Dept. of Physics, Blindern, N-0316 Oslo, Norway.
* To whom correspondence should be addressed.
D. A. Gurnett , E-mail: donald-gurnett{at}uiowa.edu
Results from the Cassini radio and plasma wave instrument arepresented during the approach and first orbit at Saturn. Duringthe approach radio emissions from Saturn showed that the radiorotation period is now 10 hours 45 min 45 ± 36 s, about6 min longer than measured by Voyager in 1980-81. Many intenseimpulsive radio signals were detected from Saturn lightningduring the approach and first orbit. Some of these have beenlinked to storm systems observed by the Cassini imaging instrument.Within the magnetosphere whistler-mode auroral hiss emissionswere observed near the rings, suggesting that a strong electrodynamicinteraction is occurring in or near the rings.
The editors suggest the following Related Resources on Science sites:
In Science Magazine
INTRODUCTION TO SPECIAL ISSUE
Linda Rowan (25 February 2005) Science307 (5713), 1222.
[DOI: 10.1126/science.307.5713.1222] |Summary »|PDF »
THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Polar Lightning and Decadal-Scale Cloud Variability on Jupiter.
K. H. Baines, A. A. Simon-Miller, G. S. Orton, H. A. Weaver, A. Lunsford, T. W. Momary, J. Spencer, A. F. Cheng, D. C. Reuter, D. E. Jennings, et al. (2007)
Science
318, 226-229
|Abstract »|Full Text »|PDF »
The Variable Rotation Period of the Inner Region of Saturn's Plasma Disk.
D. A. Gurnett, A. M. Persoon, W. S. Kurth, J. B. Groene, T. F. Averkamp, M. K. Dougherty, and D. J. Southwood (2007)
Science
316, 442-445
|Abstract »|Full Text »|PDF »
Does Enceladus govern magnetospheric dynamics at Saturn?.
Enceladus' varying imprint on the magnetosphere of Saturn..
G. H. Jones, E. Roussos, N. Krupp, C. Paranicas, J. Woch, A. Lagg, D. G. Mitchell, S. M. Krimigis, and M. K. Dougherty (2006)
Science
311, 1412-1415
|Abstract »|Full Text »|PDF »
Cassini Measurements of Cold Plasma in the Ionosphere of Titan.
J.-E. Wahlund, R. Bostrom, G. Gustafsson, D. A. Gurnett, W. S. Kurth, A. Pedersen, T. F. Averkamp, G. B. Hospodarsky, A. M. Persoon, P. Canu, et al. (2005)
Science
308, 986-989
|Abstract »|Full Text »|PDF »
Cassini Imaging Science: Initial Results on Saturn's Atmosphere.
C. C. Porco, E. Baker, J. Barbara, K. Beurle, A. Brahic, J. A. Burns, S. Charnoz, N. Cooper, D. D. Dawson, A. D. Del Genio, et al. (2005)
Science
307, 1243-1247
|Abstract »|Full Text »|PDF »
Oxygen Ions Observed Near Saturn's A Ring.
J. H. Waite Jr., T. E. Cravens, W.-H. Ip, W. T. Kasprzak, J. G. Luhmann, R. L. McNutt, H. B. Niemann, R. V. Yelle, I. Mueller-Wodarg, S. A. Ledvina, et al. (2005)
Science
307, 1260-1262
|Abstract »|Full Text »|PDF »
Composition and Dynamics of Plasma in Saturn's Magnetosphere.
D. T. Young, J.-J. Berthelier, M. Blanc, J. L. Burch, S. Bolton, A. J. Coates, F. J. Crary, R. Goldstein, M. Grande, T. W. Hill, et al. (2005)
Science
307, 1262-1266
|Abstract »|Full Text »|PDF »