Cloud-scale Turbulence
Cloud-Scale Turbulence is a physical phenomenon in astrophysical fluid dynamics characterized by chaotic, supersonic motions within interstellar molecular clouds, distinguished from other regimes of turbulence by its confinement to spatial scales of individual star-forming clouds and its dominant role in regulating cloud structure, dynamics, and star formation processes.
211
Publications
15.3K
Citations
614
Authors
300
Institutions
Publications per year
2017–2026
47
211
The Universality of Turbulence in Galactic Molecular Clouds
M. H. Heyer, Christopher M. Brunt · The Astrophysical Journal · 2004 · 487 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 211
614
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Universidad Nacional Autónoma de México, Mexico
7 publications · 1.2K citations
7
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7
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7
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1–5 of 614
300
Heidelberg University
Heidelberg, Germany
11 h-index
27 publications
2.6K citations

Centre National de la Recherche Scientifique
Paris, France
11 h-index
26 publications
2.4K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
10 h-index
23 publications
2.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
10 h-index
25 publications
1.6K citations

Australian National University
Canberra, Australia
9 h-index
15 publications
650 citations

NSF National Center for Atmospheric Research
Boulder, United States
9 h-index
13 publications
1.4K citations
G & A Technical Software (United States)
Newport News, United States
8 h-index
19 publications
572 citations
University of Maryland, College Park
College Park, United States
8 h-index
11 publications
969 citations
1–8 of 300
ApJ · 59 publications · 5.3K citations
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31 publications · 1.7K citations
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11 publications · 523 citations
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8 publications · 710 citations
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8 publications · 552 citations
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