Dust Grain Alignment

Dust Grain Alignment is a physical mechanism in astrophysics that describes the process by which non-spherical interstellar dust grains acquire a preferential orientation with respect to the magnetic field or radiation anisotropy, enabling polarization of emitted or scattered light.

160

Publications

10.6K

Citations

553

Authors

295

Institutions

Publications per year

2017–2026

61

Authors

553

  1. TH
    Thiem Hoang

    Korea Astronomy and Space Science Institute, South Korea

    15 publications · 629 citations

    14

    h-index

  2. AL
    A. Lazarian

    University of Wisconsin–Madison, United States

    11 publications · 1.2K citations

    11

    h-index

  3. BT
    B. T. Draine

    Princeton University, United States

    7 publications · 1.2K citations

    7

    h-index

  4. VG
    V. Guillet

    Centre National de la Recherche Scientifique, France

    7 publications · 625 citations

    7

    h-index

  5. PG
    P. G. Martin

    University of Toronto, Canada

    5 publications · 669 citations

    5

    h-index

1–5 of 553

Venues

  1. The Astrophysical Journal

    ApJ · 64 publications · 4.8K citations

    37

    h-index

  2. 17

    h-index

  3. Astronomy and Astrophysics

    20 publications · 1.3K citations

    16

    h-index

  4. Icarus

    7 publications · 305 citations

    7

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 103 citations

    5

    h-index

1–5