Pulsar Beam Geometry

Pulsar Beam Geometry is a theoretical construct in pulsar astronomy that characterizes the spatial configuration and emission pattern of relativistic radiation beams emanating from a neutron star’s magnetic poles, defining their angular extent, polarization properties, and viewing orientation relative to the observer.

120

Publications

8.4K

Citations

395

Authors

199

Institutions

Publications per year

2017–2026

15

Authors

395

  1. SJ
    S. Johnston

    Commonwealth Scientific and Industrial Research Organisation, Australia

    9 publications · 626 citations

    9

    h-index

  2. MK
    M. Krämer

    University of Manchester, United Kingdom

    8 publications · 454 citations

    8

    h-index

  3. JM
    Joanna M. Rankin

    University of Vermont, United States

    7 publications · 787 citations

    7

    h-index

  4. PW
    P. Weltevrede

    University of Manchester, United Kingdom

    6 publications · 437 citations

    6

    h-index

  5. UK
    U. Kraus

    University of Tübingen, Germany

    6 publications · 209 citations

    6

    h-index

1–5 of 395

Venues

  1. The Astrophysical Journal

    ApJ · 48 publications · 3.5K citations

    28

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    35 publications · 2.8K citations

    24

    h-index

  3. Astronomy and Astrophysics

    4 publications · 161 citations

    4

    h-index

  4. Nature

    4 publications · 298 citations

    4

    h-index

  5. Advances in Space Research

    2 publications · 68 citations

    2

    h-index

1–5