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Large-scale horizontal flows in the solar photosphere IV. On the vertical structure of large-scale horizontal flows

✍ Scribed by M. Švanda; M. Klvaňa; M. Sobotka; A.G. Kosovichev; T.L. Duvall Jr.

Publisher
Elsevier Science
Year
2009
Tongue
English
Weight
726 KB
Volume
14
Category
Article
ISSN
1384-1076

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✍ W.J. Layton 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 115 KB

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