Damping Processes

Damping Processes is a physical mechanism within the study of pulsating stars that describes the dissipation of pulsational energy through radiative losses, turbulent viscosity, or non-adiabatic effects, thereby reducing the amplitude of stellar oscillations over time.

216

Publications

9.4K

Citations

672

Authors

294

Institutions

Publications per year

2017–2026

35

Authors

672

  1. KB
    K. Belkacem

    Laboratoire d’études spatiales et d’instrumentation en astrophysique, France

    4 publications · 148 citations

    4

    h-index

  2. ED
    E. D. Fredrickson

    Princeton Plasma Physics Laboratory, United States

    3 publications · 118 citations

    3

    h-index

  3. AB
    A. Biancalani

    Max Planck Institute for Plasma Physics, Germany

    3 publications · 82 citations

    3

    h-index

  4. MG
    M. Goossens

    KU Leuven, Belgium

    3 publications · 233 citations

    3

    h-index

  5. FZ
    F. Zonca

    National Agency for New Technologies, Energy and Sustainable Economic Development, Italy

    3 publications · 70 citations

    3

    h-index

1–5 of 672

Venues

  1. Physics of Plasmas

    17 publications · 634 citations

    15

    h-index

  2. Physical Review Letters

    PRL · 12 publications · 922 citations

    12

    h-index

  3. 11

    h-index

  4. The Astrophysical Journal

    ApJ · 9 publications · 394 citations

    10

    h-index

  5. Nuclear Fusion

    11 publications · 253 citations

    10

    h-index

1–5