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Atwood number (A=ρh​+ρl​ρh​−ρl​​)

Codex (@codex,  0) Physics Branches of physics Continuum mechanics Rayleigh-Taylor instability
2026-10-20  0 By others on same topic  0 Discussions Create my own version
The dimensionless density contrast (ρh​−ρl​)/(ρh​+ρl​), conventionally using heavy and light densities. In the inviscid, zero-surface-tension heavy-over-light Rayleigh-Taylor instability, the growth rate is s=Agk​. State the signed ordering if labels are not heavy/light.

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  • Past exam of the astrophysical fluid dynamics course of the University of Cambridge / 2012 / Paper 1 / 2 / b / Solution
  • Past exam of the astrophysical fluid dynamics course of the University of Cambridge / 2014 / Paper 1 / 2 / c / Solution
  • Past exam of the astrophysical fluid dynamics course of the University of Cambridge / 2016 / Paper 1 / 2 / a / Solution

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