Turbulence Decay

Turbulence Decay is a physical process in astrophysical fluid dynamics characterized by the gradual dissipation of turbulent kinetic energy in interstellar media due to viscous and resistive effects, leading to a reduction in velocity fluctuations and magnetic field perturbations over time.

690

Publications

43.2K

Citations

1.2K

Authors

575

Institutions

Publications per year

2017–2026

96

Authors

1.2K

  1. RA
    R. A. Antonia

    University of Newcastle Australia, Australia

    24 publications · 998 citations

    18

    h-index

  2. AB
    Axel Brandenburg

    Stockholm University, Sweden

    16 publications · 1.2K citations

    14

    h-index

  3. LD
    L. Djenidi

    University of Newcastle Australia, Australia

    13 publications · 557 citations

    13

    h-index

  4. LD
    Luminita Danaila

    Complexe de Recherche Interprofessionnel en Aérothermochimie, France

    14 publications · 460 citations

    13

    h-index

  5. ZW
    Z. Warhaft

    Cornell University, United States

    12 publications · 1.7K citations

    12

    h-index

1–5 of 1.2K

Venues

  1. Journal of Fluid Mechanics

    108 publications · 9.1K citations

    49

    h-index

  2. Physics of Fluids

    94 publications · 5.3K citations

    40

    h-index

  3. Physical Review Letters

    PRL · 40 publications · 3.9K citations

    34

    h-index

  4. The Astrophysical Journal

    ApJ · 30 publications · 2.4K citations

    20

    h-index

  5. The Physics of Fluids

    30 publications · 1.7K citations

    18

    h-index

1–5