Pulsar Interstellar Scattering

Pulsar Interstellar Scattering is a physical phenomenon in pulsar astronomy characterized by the distortion of pulsed radio emission due to multipath propagation caused by density inhomogeneities in the interstellar medium, leading to temporal broadening and intensity fluctuations of the observed signal.

183

Publications

10.6K

Citations

545

Authors

210

Institutions

Publications per year

2017–2026

38

Variants

Interstellar Scattering Of Pulsars

Authors

545

  1. JM
    J. M. Cordes

    Cornell University, United States

    18 publications · 2.9K citations

    17

    h-index

  2. DR
    Daniel R. Stinebring

    Oberlin College, United States

    18 publications · 792 citations

    15

    h-index

  3. MK
    M. Krämer

    University of Manchester, United Kingdom

    10 publications · 450 citations

    10

    h-index

  4. SM
    S. M. Ransom

    National Radio Astronomy Observatory, United States

    10 publications · 989 citations

    10

    h-index

  5. DR
    D. R. Lorimer

    West Virginia University, United States

    9 publications · 1.2K citations

    9

    h-index

1–5 of 545

Venues

  1. The Astrophysical Journal

    ApJ · 73 publications · 5.9K citations

    38

    h-index

  2. 27

    h-index

  3. Astronomy and Astrophysics

    12 publications · 538 citations

    12

    h-index

  4. 4

    h-index

  5. Nature

    3 publications · 112 citations

    3

    h-index

1–5