In many geophysical fluid modeling applications there exist two very different time scales, essentially fast waves and slow vortices. At the largest planetary scales inertialgravity waves propagate through the fluid at phase speeds much faster than particle velocities, while at small scales fast aco
✦ LIBER ✦
VLES modelling of geophysical fluids with nonoscillatory forward-in-time schemes
✍ Scribed by P. K. Smolarkiewicz; J. M. Prusa
- Publisher
- John Wiley and Sons
- Year
- 2002
- Tongue
- English
- Weight
- 305 KB
- Volume
- 39
- Category
- Article
- ISSN
- 0271-2091
- DOI
- 10.1002/fld.330
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2.2.2, the invariant I 3 was mistakenly identified as 'the third invariant of the Green-Lagrange strain tensor.' It should have been identified as 'the third invariant of the right Cauchy-Green deformation tensor.' The computation reported in the paper was based on that. In Section 4.1.2, the expon