Dynamics, Composition, and Origin of Jovian and Saturnian Dust-Stream Particles

Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 385)

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.

Keywords

Solar Wind Dust Particle Interplanetary Magnetic Field Stream Particle Dust Flux 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  • Hsiang-Wen Hsu
    • 1
  • Harald Krüger
    • 2
    • 3
  • Frank Postberg
    • 3
    • 4
  1. 1.Laboratory for Atmospheric and Space PhysicsUniversity of ColoradoBoulderUSA
  2. 2.Max-Planck-Institut für SonnensystemforschungKatlenburg-LindauGermany
  3. 3.Max-Planck-Institut für KernphysikHeidelbergGermany
  4. 4.Institut für GeowissenschaftenRuprecht-Karls UniversitätHeidelbergGermany

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