Abstract
Stream particles are nanometer-sized dust particles ejected from the Jovian and Saturnian systems with speeds higher than 100\(\mathrm{{km\,s}}^{-1}\). Due to the large charge-to-mass ratio, their dynamics is dominated by electromagnetic forces, which lead to the high-speed ejection from the planetary magnetospheres and the dust impact bursts reported from the in situ dust measurements (i.e., the dust stream phenomena). Following measurements with the in situ dust detectors on board the Ulysses, Galileo, and Cassini spacecrafts, we summarize the sources as well as the dynamical and compositional properties of these nanoparticles. Future stream particle studies should focus on the connection between dust, moons, and the magnetosphere.
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Notes
- 1.
Due to a mixup of size and radius, the values given here are two times smaller than in the original publication.
- 2.
The time between the release of a particle into the magnetosphere and its ejection from the system.
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Hsu, HW., Krüger, H., Postberg, F. (2012). Dynamics, Composition, and Origin of Jovian and Saturnian Dust-Stream Particles. In: Mann, I., Meyer-Vernet, N., Czechowski, A. (eds) Nanodust in the Solar System: Discoveries and Interpretations. Astrophysics and Space Science Library, vol 385. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27543-2_5
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