2015
DOI: 10.1016/j.icarus.2015.03.019
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Three-dimensional simulation of gas and dust in Io’s Pele plume

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Cited by 20 publications
(12 citation statements)
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“…If supersonic vents generate the plumes, the reduced height of a shocked plume and the increased number densities in the canopy correspond well with current observations ( Roth et al, 2014a ). This suggests a single large vent ( D vent = ∼74 m) or many small vents located very close together ( McDoniel et al, 2015 ) are reasonable configurations. In both cases the total mass flow would be on the order of 10 0 0 kg/s.…”
Section: Discussionmentioning
confidence: 88%
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“…If supersonic vents generate the plumes, the reduced height of a shocked plume and the increased number densities in the canopy correspond well with current observations ( Roth et al, 2014a ). This suggests a single large vent ( D vent = ∼74 m) or many small vents located very close together ( McDoniel et al, 2015 ) are reasonable configurations. In both cases the total mass flow would be on the order of 10 0 0 kg/s.…”
Section: Discussionmentioning
confidence: 88%
“…Due to the wedge-shaped domain, cells nearest the symmetry axis have very small volumes and therefore contain relatively few computational particles, leading to poor statistics for cell-averaged quantities. Boosting the number of simulated particles or employing weighting schemes mitigates this effect ( McDoniel et al, 2015 ).…”
Section: Stagingmentioning
confidence: 99%
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“…4. Particle Balancing (perhaps first applied to DSMC in [9] and used in codes like UT's PLANET [12] or Sandia's SPARTA [http://sparta.sandia.gov]): Another popular balancing method uses particle count as a proxy for load. Processor boundaries are drawn such that each processor owns space containing roughly equal numbers of particles.…”
Section: State Of the Artmentioning
confidence: 99%
“…Using this qualitative analogy, I proposed that umbrella-shaped plumes, such as those from Pele or Prometheus, were pressure balanced and that the irregularly shaped plumes, such as the one that erupted from Loki, were overpressured (Kieffer 1982a). Continued observations over the decades have produced higher-resolution data about the structure and temporal behavior of the Ionian plumes, and models using ever more sophisticated supercomputer simulations have been able to incorporate rarefied gas dynamics, phase changes, particle loading, and three-dimensional vent geometries to explain plume structure (e.g., McDoniel et al 2015).…”
Section: Laval Nozzlesmentioning
confidence: 99%