The truncation error of the rotational form for the convective terms in the Navier-Stokes equation is examined in the direct numerical simulation (DNS) of the fully developed turbulent channel flow, in which the low-order finite difference method was used for the partial derivatives in the wall-norm
β¦ LIBER β¦
New form of dynamo equation for convective regions of rotating stars
β Scribed by G. S. Bisnovatyi-Kogan
- Publisher
- Springer Netherlands
- Year
- 1992
- Tongue
- English
- Weight
- 135 KB
- Volume
- 189
- Category
- Article
- ISSN
- 0004-640X
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