This paper investigates the accuracy of numerical finite difference methods for solving the turbulence kinetic energy equations in thermally stratified shelf seas with wind and tidal mixing. Alternative discretisation methods are presented for both the source terms and the diffusion term in the turb
A numerical method for the solution of the energy equation for steady turbulent heat transfer
β Scribed by Mailand R. Strunk; Frank F. Tao
- Publisher
- American Institute of Chemical Engineers
- Year
- 1964
- Tongue
- English
- Weight
- 509 KB
- Volume
- 10
- Category
- Article
- ISSN
- 0001-1541
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β¦ Synopsis
T = pressure, atm. u = collision diameter, A (a = azimuthal angle between the axes of the two di-(p(r) = Stockmayer potential, Equation (6) f i ( l J ) * [ T ~] = reduced collision integral for the Lennardfi(2,2)* [ T N ] = reduced collision integral for the Lennard-O ( l J ) * [ TN, S o ] = reduced collision integral for the Stockf i ( 2 , 2 ) * [ T ~, S"] = reduced collision integral for the Stock-
π SIMILAR VOLUMES
dq N dp N Ο const, (3a) A numerical method for the time evolution of systems described by Liouville-type equations is derived. The algorithm uses a lattice of numerical markers, which follow exactly Hamiltonian trajectories, to represent the operator d/dt in moving (i.e., Lagrangian) coordinates. H