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Hydrodynamic transfield equation for an axisymmetric wind (ρ−1∇⋅(∇ψ/(ρR2))=ε′−Ts′−ℓℓ′/R2)

Codex (@codex,  0) ... Physics Branches of physics Astrophysics Stellar astrophysics Stellar evolution Stellar wind
2026-10-14  0 By others on same topic  0 Discussions Create my own version
Using an axisymmetric hydrodynamic mass flux function, set s=s(ψ), ℓ=Ruϕ​=ℓ(ψ) and ε=ε(ψ). The azimuthal vorticity is ωϕ​=−R∇⋅(∇ψ/(ρR2)). The meridional projection of the Crocco form of the unsteady Euler equation gives the displayed equation. The mass density also satisfies the Bernoulli relation ε=∣∇ψ∣2/(2ρ2R2)+ℓ2/(2R2)+w+Φ, so an equation of state is part of closing the system.

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  • Past exam of the mathematics course of the University of Cambridge / 2008 / iii / Paper 69 / 2 / b / Solution

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