Interstellar Turbulence
Interstellar Turbulence is a stochastic, multi-scale flow phenomenon within the interstellar medium characterized by chaotic motions of gas and magnetic fields that deviate from laminar behavior and significantly influence star formation, cosmic ray propagation, and the structure of galactic matter.
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2017–2026
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Rapid planetesimal formation in turbulent circumstellar disks
Anders Johansen, Jeffrey S. Oishi, Mordecai‐Mark Mac Low et al. · Nature · 2007 · 1.2K citations · Full text
Interstellar Turbulence I: Observations and Processes
Annual Review of Astronomy and Astrophysics · 2004 · 1.2K citations · Full text
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Centre National de la Recherche Scientifique
Paris, France
51 h-index
326 publications
31.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
44 h-index
114 publications
10.2K citations
University of Wisconsin–Madison
Madison, United States
41 h-index
171 publications
10.6K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
36 h-index
129 publications
18.8K citations
University of California San Diego
San Diego, United States
34 h-index
66 publications
4.4K citations
California Institute of Technology
Pasadena, United States
34 h-index
73 publications
9K citations
Université Paris Cité
Paris, France
33 h-index
118 publications
16K citations
Heidelberg University
Heidelberg, Germany
32 h-index
107 publications
10.1K citations
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ApJ · 458 publications · 41.1K citations
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233 publications · 14.7K citations
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109 publications · 9.3K citations
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37 publications · 2.1K citations
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Repository · 22 publications · 1.9K citations
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