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

Publications

20.4K

Citations

610

Authors

333

Institutions

Publications per year

2017–2026

38

Authors

610

  1. RA
    R. A. Antonia

    University of Newcastle Australia, Australia

    10 publications · 308 citations

    10

    h-index

  2. LS
    L. Skrbek

    Charles University, Czechia

    9 publications · 675 citations

    9

    h-index

  3. LD
    L. Djenidi

    University of Newcastle Australia, Australia

    9 publications · 293 citations

    9

    h-index

  4. AB
    Axel Brandenburg

    Stockholm University, Sweden

    8 publications · 446 citations

    8

    h-index

  5. RB
    Roberto Benzi

    University of Rome Tor Vergata, Italy

    6 publications · 527 citations

    6

    h-index

1–5 of 610

Venues

  1. Journal of Fluid Mechanics

    49 publications · 3.9K citations

    31

    h-index

  2. Physics of Fluids

    40 publications · 2.5K citations

    24

    h-index

  3. Physical Review Letters

    PRL · 22 publications · 2K citations

    21

    h-index

  4. The Astrophysical Journal

    ApJ · 13 publications · 1.5K citations

    12

    h-index

  5. Physics of Fluids A Fluid Dynamics

    12 publications · 1.5K citations

    12

    h-index

1–5