Solar Eigenfunctions

Solar Eigenfunctions is a mathematical construct in helioseismology that represents the spatial patterns of oscillation modes in the Sun, derived as solutions to the linearized equations of stellar pulsation under spherical symmetry and stratified structure.

79

Publications

2.9K

Citations

133

Authors

86

Institutions

Publications per year

2017–2026

8

Authors

133

  1. GR
    G. R. Isaak

    University of Birmingham, United Kingdom

    5 publications · 135 citations

    5

    h-index

  2. RN
    R. New

    Sheffield Hallam University, United Kingdom

    4 publications · 118 citations

    4

    h-index

  3. YE
    Y. Elsworth

    University of Birmingham, United Kingdom

    4 publications · 118 citations

    4

    h-index

  4. BA
    B. A. Miller

    University of Birmingham, United Kingdom

    4 publications · 118 citations

    4

    h-index

  5. MR
    M. Roth

    Institut für Sonnenphysik, Germany

    4 publications · 122 citations

    4

    h-index

1–5 of 133

Venues

  1. The Astrophysical Journal

    ApJ · 24 publications · 1.2K citations

    17

    h-index

  2. Solar Physics

    13 publications · 420 citations

    11

    h-index

  3. 10

    h-index

  4. Advances in Space Research

    4 publications · 79 citations

    4

    h-index

  5. Astronomy and Astrophysics

    4 publications · 83 citations

    4

    h-index

1–5