Accretion Disk Plasmas

Accretion Disk Plasmas is a theoretical construct representing magnetized, high-temperature plasma flows in differentially rotating circumstellar disks, distinguished by their role in mediating angular momentum transport and radiative energy conversion in astrophysical accretion systems.

1.8K

Publications

127.8K

Citations

3.7K

Authors

991

Institutions

Publications per year

2017–2026

335

Authors

3.7K

  1. RV
    R. V. E. Lovelace

    Cornell University, United States

    26 publications · 2.6K citations

    20

    h-index

  2. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    22 publications · 2.5K citations

    19

    h-index

  3. JM
    J. M. Mïller

    University of Michigan, United States

    20 publications · 1.9K citations

    18

    h-index

  4. MC
    Mitchell C. Begelman

    Joint Institute for Laboratory Astrophysics, United States

    18 publications · 1.6K citations

    17

    h-index

  5. EQ
    Eliot Quataert

    University of California, Berkeley, United States

    17 publications · 1K citations

    16

    h-index

1–5 of 3.7K

Venues

  1. The Astrophysical Journal

    ApJ · 702 publications · 61.4K citations

    119

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    251 publications · 18.4K citations

    64

    h-index

  3. Astronomy and Astrophysics

    181 publications · 8.9K citations

    52

    h-index

  4. Publications of the Astronomical Society of Japan

    48 publications · 2.3K citations

    26

    h-index

  5. The Astrophysical Journal Letters

    46 publications · 2.1K citations

    25

    h-index

1–5