Poloidal Magnetic Fields

Poloidal Magnetic Fields is a type of large-scale magnetic field configuration in astrophysical plasmas, characterized by magnetic field lines that loop from the interior of a celestial body or disk outward to the poles and back, as opposed to toroidal fields that wrap azimuthally around the equatorial plane.

1K

Publications

65.8K

Citations

3.2K

Authors

776

Institutions

Publications per year

2017–2026

175

Authors

3.2K

  1. JD
    J.‐F. Donati

    Centre National de la Recherche Scientifique, France

    12 publications · 1.3K citations

    12

    h-index

  2. GI
    Gordon I. Ogilvie

    University of Cambridge, United Kingdom

    9 publications · 773 citations

    9

    h-index

  3. KS
    Kazunari Shibata

    Kyoto University, Japan

    9 publications · 887 citations

    9

    h-index

  4. PP
    P. Petit

    Centre National de la Recherche Scientifique, France

    9 publications · 876 citations

    9

    h-index

  5. SS
    S. Schramm

    University of Oklahoma, United States

    8 publications · 271 citations

    8

    h-index

1–5 of 3.2K

Venues

  1. The Astrophysical Journal

    ApJ · 154 publications · 16.6K citations

    63

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    139 publications · 14.1K citations

    49

    h-index

  3. Nuclear Fusion

    102 publications · 4.9K citations

    37

    h-index

  4. Physics of Plasmas

    66 publications · 2.6K citations

    28

    h-index

  5. Astronomy and Astrophysics

    42 publications · 2.4K citations

    28

    h-index

1–5