Pulsar Magnetic Fields

Pulsar Magnetic Fields is a theoretical construct representing the highly intense, dynamically evolving electromagnetic field structures generated by and intrinsic to neutron stars exhibiting periodic pulsed emission, distinguished from other stellar magnetic fields by their extreme strength, rapid rotation-induced field line geometry, and central role in powering relativistic particle acceleration and coherent radio emission mechanisms.

932

Publications

63.4K

Citations

1.8K

Authors

597

Institutions

Publications per year

2017–2026

145

Authors

1.8K

  1. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    26 publications · 2.2K citations

    22

    h-index

  2. VM
    V. M. Kaspi

    McGill University, Canada

    24 publications · 2.9K citations

    22

    h-index

  3. AK
    A. K. Harding

    Goddard Space Flight Center, United States

    25 publications · 1.9K citations

    21

    h-index

  4. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    20 publications · 2.3K citations

    19

    h-index

  5. MK
    M. Krämer

    University of Manchester, United Kingdom

    21 publications · 1.6K citations

    19

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 294 publications · 28K citations

    84

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    168 publications · 8.9K citations

    52

    h-index

  3. Astronomy and Astrophysics

    41 publications · 2K citations

    27

    h-index

  4. The Astrophysical Journal Letters

    28 publications · 2K citations

    23

    h-index

  5. Nature

    27 publications · 3.5K citations

    19

    h-index

1–5