Driven Turbulence

Driven Turbulence is a type of turbulence in star-forming regions characterized by the sustained injection of kinetic energy through external or internal mechanisms, such as stellar feedback or large-scale gravitational flows, that actively maintain turbulent motions against dissipative processes.

115

Publications

7.5K

Citations

343

Authors

223

Institutions

Publications per year

2017–2026

22

Variants

Forced Turbulence

Authors

343

  1. CH
    Ch. Helling

    University of St Andrews, United Kingdom

    6 publications · 704 citations

    6

    h-index

  2. PW
    P. Woitke

    University of St Andrews, United Kingdom

    5 publications · 616 citations

    5

    h-index

  3. SB
    Stanislav Boldyrev

    University of Wisconsin–Madison, United States

    3 publications · 429 citations

    3

    h-index

  4. ES
    E. Sedlmayr

    Technische Universität Berlin, Germany

    3 publications · 160 citations

    3

    h-index

  5. MC
    Mitchell C. Begelman

    Joint Institute for Laboratory Astrophysics, United States

    3 publications · 301 citations

    3

    h-index

1–5 of 343

Venues

  1. The Astrophysical Journal

    ApJ · 27 publications · 2.1K citations

    23

    h-index

  2. 13

    h-index

  3. Astronomy and Astrophysics

    12 publications · 1.2K citations

    12

    h-index

  4. Physics of Plasmas

    10 publications · 564 citations

    10

    h-index

  5. Physical Review Letters

    PRL · 8 publications · 722 citations

    8

    h-index

1–5