Magnetic Field Evolution

Magnetic Field Evolution is a theoretical framework that describes the temporal changes in magnetic field configurations across astrophysical scales—from planetary and stellar interiors to interstellar and galactic environments—by modeling the dynamical processes such as flux freezing, magnetic reconnection, and magnetohydrodynamic turbulence that govern the generation, amplification, and dissipation of magnetic fields.

1.3K

Publications

83.8K

Citations

2.9K

Authors

974

Institutions

Publications per year

2017–2026

260

Authors

2.9K

  1. LF
    L. F. Burlaga

    Goddard Space Flight Center, United States

    16 publications · 2.2K citations

    16

    h-index

  2. AB
    Axel Brandenburg

    Stockholm University, Sweden

    16 publications · 1.2K citations

    15

    h-index

  3. DM
    D. Moss

    University of Manchester, United Kingdom

    13 publications · 397 citations

    12

    h-index

  4. JA
    J. A. Pons

    University of Alicante, Spain

    12 publications · 775 citations

    12

    h-index

  5. CT
    C. T. Russell

    University of California, Los Angeles, United States

    14 publications · 908 citations

    12

    h-index

1–5 of 2.9K

Venues

  1. The Astrophysical Journal

    ApJ · 286 publications · 20.3K citations

    80

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    190 publications · 9.7K citations

    53

    h-index

  3. Astronomy and Astrophysics

    106 publications · 7.2K citations

    47

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 53 publications · 5.2K citations

    36

    h-index

  5. Physical Review Letters

    PRL · 31 publications · 2.2K citations

    24

    h-index

1–5