Synchrotron Polarization

Synchrotron Polarization is a radiative process in which relativistic electrons gyrating around magnetic field lines emit linearly polarized radiation due to the anisotropic distribution of their trajectories, thereby serving as a key observational tracer of magnetic field orientation and strength in astrophysical plasmas.

196

Publications

9.4K

Citations

652

Authors

251

Institutions

Publications per year

2017–2026

37

Authors

652

  1. AL
    A. Lazarian

    University of Wisconsin–Madison, United States

    8 publications · 219 citations

    8

    h-index

  2. EC
    E. Carretti

    Commonwealth Scientific and Industrial Research Organisation, Australia

    6 publications · 151 citations

    6

    h-index

  3. TW
    T. W. Jones

    University College London, United Kingdom

    5 publications · 524 citations

    5

    h-index

  4. RB
    R. Beck

    Max Planck Institute for Radio Astronomy, Germany

    5 publications · 217 citations

    5

    h-index

  5. TR
    T. Roser

    Brookhaven National Laboratory, United States

    4 publications · 155 citations

    4

    h-index

1–5 of 652

Venues

  1. The Astrophysical Journal

    ApJ · 55 publications · 3.5K citations

    32

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.5K citations

    20

    h-index

  3. Physical Review Letters

    PRL · 11 publications · 494 citations

    11

    h-index

  4. Review of Scientific Instruments

    9 publications · 256 citations

    9

    h-index

  5. 7

    h-index

1–5