Literature DB >> 15604362

Radio and plasma wave observations at Saturn from Cassini's approach and first orbit.

D A Gurnett1, W S Kurth, G B Hospodarsky, A M Persoon, T F Averkamp, B Cecconi, A Lecacheux, P Zarka, P Canu, N Cornilleau-Wehrlin, P Galopeau, A Roux, C Harvey, P Louarn, R Bostrom, G Gustafsson, J-E Wahlund, M D Desch, W M Farrell, M L Kaiser, K Goetz, P J Kellogg, G Fischer, H-P Ladreiter, H Rucker, H Alleyne, A Pedersen.   

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.

Year:  2004        PMID: 15604362     DOI: 10.1126/science.1105356

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Saturn's fast spin determined from its gravitational field and oblateness.

Authors:  Ravit Helled; Eli Galanti; Yohai Kaspi
Journal:  Nature       Date:  2015-03-25       Impact factor: 49.962

  1 in total

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