Granular Matter Group Members
Astrophysics Nonlinear Dynamics Group
Planetary Rings/Dust Dynamics  

Granular Matter

Examples:

  • cosmic:
    • planetary rings
    • protoplanetary discs/planetary evolution
    • clouds/discs of gas and dust
  • terrestrial:
    • avalanches
    • dunes
    • sandpiles
    • fields of drift ice

Physical Processes:


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Astrophysics

Planetary Rings:

  • undisturbed rings:
    • kinetic/hydrodynamic description
    • vertical structure
    • processes of transport
    • instabilities/structures
  • perturbed rings:
    • waves and resonances
    • moonlets in rings
    • e.g. satellite Pan in Saturn's A ring

Planetogony/Planet Formation:

  • from planetesimals to planets
  • interaction of a planet with a protoplanetary disc

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Interplanetary Dust Dynamics:

Cassini Project

  • Participation in Spaceprobe Experiments:
    • dustdetection:
      • spaceprobe Galileo: DDS (Dust Detector System)
      • spaceprobe Cassini: CDA (Cosmic Dust Analyzer)
      • spaceprobe Ulysses: DDS
    • ultraviolett spectroscopy:
      • spaceprobe Cassini: UVIS (Ultra-Violet-Imaging-Spectrometer)
  • Modelling of Dustconfigurations:
    • Tori of Dust around Mars
    • Population of Dust at Jupiter/rings of Jupiter
    • Dustatmospheres of Saturns rings/ Saturns E ring/the "Spokes"-phenonemen
    • Enceladus' Geysers and -Dust Plume: Main Source of the E Ring of Saturn
  • Structure-formations in Dense Planetary Rings:
    • Propeller-Structuctures caused by kilometer-sized Moonlets in Dense Rings
    • Non-linear Diffusion, Angular-Momentum Flux reversals, and sharp Ring-Edges created by Ring-Moons
    • Instabilities and related spontaneous Structures - ``Overstability'' and more
    • Kinetics of Aggregation, Restitution, and Fragmentation

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Last modified: Wed March 17; 17:00:29 CEST 2021