4.4 Article

Observation of the spatial growth of self-excited dust-density waves

Journal

PHYSICS OF PLASMAS
Volume 17, Issue 12, Pages -

Publisher

AIP Publishing
DOI: 10.1063/1.3524691

Keywords

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Funding

  1. NASA [NNX07AD22G, NNX10AR55G]
  2. NSF [0903501]
  3. Direct For Mathematical & Physical Scien
  4. Division Of Physics [0923141] Funding Source: National Science Foundation
  5. Division Of Physics
  6. Direct For Mathematical & Physical Scien [0903501] Funding Source: National Science Foundation
  7. NASA [NNX10AR55G, 124260] Funding Source: Federal RePORTER

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The growth of a naturally occurring dust-density wave (DDW) is experimentally observed using high-speed imaging. This low frequency wave (similar to 25 Hz) grows in amplitude as it propagates downward through a dusty plasma. The wave's linear growth rate -k(i) is measured using a phase-sensitive analysis method. For the conditions studied here, the growth rate increases as gas pressure decreases. At a critical gas pressure, which is observed, a balance between an ion-flow instability and dissipation by neutral gas drag determines a threshold for wave propagation. A linear dispersion relation is derived, taking into account the effects of strong-coupling, to compare to the experiment. (C) 2010 American Institute of Physics. [doi: 10.1063/1.3524691]

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