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| | Possible sources for the Saturnian dust streams |
 | | In this work we apply an analytical model, already applied to Jupiter (Maravilla et al., 1995), in order to analyze two possible and different sources: On the one hand the satellites Dione, Helene, Rhea and Enceladus; on the second, the A-ring outer boundary. |
 | | Additionally, some general properties of the dust particles that compose these Saturnian streams, such as their radii and escaping speeds, are drawn. |
 | | Citation: Maravilla, D., and A. Flandes (2005), Possible sources for the Saturnian dust streams, Geophys. |
| www.agu.org /pubs/crossref/2005/2004GL021842.shtml (221 words) |
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