The Enceladus satellite as a source of N+ ions in Saturn's magnetosphere
The first pass of the Cassini probe in the vicinity of Saturn, above the E- ring, demonstrated a plasma consisting of water group ions (H+, O+, OH+, H2O+) with a small N+ ion component (3%). Using a simple model for the transport of magnetospheric ions, we show that the N+ ions can be traced back to...
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| Published in | Comptes rendus. Physique Vol. 6; no. 10; pp. 1176 - 1181 |
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| Main Authors | , , , , , , |
| Format | Journal Article |
| Language | English French |
| Published |
01.01.2005
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| Online Access | Get full text |
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| Abstract | The first pass of the Cassini probe in the vicinity of Saturn, above the E- ring, demonstrated a plasma consisting of water group ions (H+, O+, OH+, H2O+) with a small N+ ion component (3%). Using a simple model for the transport of magnetospheric ions, we show that the N+ ions can be traced back to the Enceladus satellite. Such a result can be explained by the existence in this icy satellite, supposed to be still geologically active, of volatile components such as ammonia NH3, or by the previous implantation of N+ ions of external origin on its surface. To cite this article: M. Bouhram et al., C. R. Physique 6 (2005). |
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| AbstractList | The first pass of the Cassini probe in the vicinity of Saturn, above the E- ring, demonstrated a plasma consisting of water group ions (H+, O+, OH+, H2O+) with a small N+ ion component (3%). Using a simple model for the transport of magnetospheric ions, we show that the N+ ions can be traced back to the Enceladus satellite. Such a result can be explained by the existence in this icy satellite, supposed to be still geologically active, of volatile components such as ammonia NH3, or by the previous implantation of N+ ions of external origin on its surface. To cite this article: M. Bouhram et al., C. R. Physique 6 (2005). |
| Author | Bouhram, Mehdi Smith, Howard T Sittler, Edward C Illiano, Jean-Marie Berthelier, Jean-Jacques Crary, Frank J Young, Dave T |
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