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The possible protogalactic role of eddies in a turbulent early universe

✍ Scribed by Wilbur K. Brown


Publisher
Springer Netherlands
Year
1985
Tongue
English
Weight
416 KB
Volume
115
Category
Article
ISSN
0004-640X

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In turbulent flow, the normal procedure has been to seek means u of the fluid velocity u rather than the velocity itself. If these means are defined by local spacial averaging with an averaging radius of ␦ the approach is known as large eddy Ž . simulation, and u denotes the eddies of size 0 ␦ and l