Decaying Turbulence
Decaying Turbulence is a theoretical construct in astrophysical fluid dynamics denoting the temporal dissipation of supersonic turbulent motions in star-forming regions due to the absence of external driving forces, leading to a progressive reduction in kinetic energy and turbulence support against gravitational collapse.
311
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20.4K
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610
Authors
333
Institutions
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2017–2026
38
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Turbulence: an introduction for scientists and engineers
Choice Reviews Online · 2005 · 1.1K citations
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Centre National de la Recherche Scientifique
Paris, France
23 h-index
59 publications
2.9K citations
University of Cambridge
Cambridge, United Kingdom
13 h-index
23 publications
2.2K citations
University of Newcastle Australia
Newcastle, Australia
11 h-index
30 publications
985 citations
Observatoire de la Côte d’Azur
Nice, France
10 h-index
14 publications
1.2K citations
Charles University
Prague, Czechia
8 h-index
16 publications
547 citations

NSF National Center for Atmospheric Research
Boulder, United States
8 h-index
18 publications
1.1K citations
Princeton University
Princeton, United States
8 h-index
12 publications
1K citations

Sorbonne Université
Paris, France
7 h-index
15 publications
888 citations
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49 publications · 3.9K citations
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40 publications · 2.5K citations
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PRL · 22 publications · 2K citations
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ApJ · 13 publications · 1.5K citations
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12 publications · 1.5K citations
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