Pulsar Polarization

Pulsar Polarization is a polarimetric phenomenon characterized by the ordered orientation of electromagnetic wave electric fields in the emission beams of rotating neutron stars, distinguished from other astrophysical polarization sources by its periodic modulation and intrinsic connection to the pulsar’s magnetic geometry and radiation mechanism.

489

Publications

26.2K

Citations

2.2K

Authors

498

Institutions

Publications per year

2017–2026

105

Authors

2.2K

  1. SJ
    S. Johnston

    Commonwealth Scientific and Industrial Research Organisation, Australia

    45 publications · 2.4K citations

    32

    h-index

  2. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    32 publications · 3.3K citations

    27

    h-index

  3. JM
    Joanna M. Rankin

    University of Vermont, United States

    32 publications · 1.9K citations

    24

    h-index

  4. AK
    A. Karastergiou

    University of Oxford, United Kingdom

    28 publications · 1.2K citations

    22

    h-index

  5. MK
    M. Krämer

    University of Manchester, United Kingdom

    27 publications · 1.3K citations

    22

    h-index

1–5 of 2.2K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    138 publications · 7.6K citations

    49

    h-index

  2. The Astrophysical Journal

    ApJ · 135 publications · 8K citations

    49

    h-index

  3. Astronomy and Astrophysics

    31 publications · 1.3K citations

    24

    h-index

  4. Nature

    15 publications · 1.8K citations

    13

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 9 publications · 298 citations

    9

    h-index

1–5