Magnetohydrodynamic Disk Effects

Magnetohydrodynamic Disk Effects is a theoretical framework in astrophysical fluid dynamics that describes the influence of magnetic fields and ionized gas interactions on the structure and evolution of protoplanetary disks, thereby modulating the angular momentum transport and migration pathways of embedded planets.

45

Publications

3.5K

Citations

125

Authors

123

Institutions

Publications per year

2017–2026

11

Authors

125

  1. SC
    S. Cabrit

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    2 publications · 151 citations

    2

    h-index

  2. JP
    J. P. Cassinelli

    University of Wisconsin–Madison, United States

    2 publications · 102 citations

    2

    h-index

  3. DC
    D. C. Telfer

    University of Wisconsin–Madison, United States

    2 publications · 102 citations

    2

    h-index

  4. MM
    M. M. Romanova

    Cornell University, United States

    2 publications · 309 citations

    2

    h-index

  5. EB
    E. Bianchi

    Université Grenoble Alpes, France

    2 publications · 151 citations

    2

    h-index

1–5 of 125

Venues

  1. The Astrophysical Journal

    ApJ · 10 publications · 878 citations

    10

    h-index

  2. Astronomy and Astrophysics

    6 publications · 556 citations

    6

    h-index

  3. 6

    h-index

  4. The Astrophysical Journal Letters

    4 publications · 125 citations

    4

    h-index

  5. Astrophysics and Space Science

    3 publications · 123 citations

    3

    h-index

1–5