Solar Spin-down

Solar Spin-Down is a theoretical construct in solar astrophysics denoting the gradual reduction in the Sun's angular momentum over time due to magnetized stellar wind torque, distinguishing it from other rotational evolution mechanisms by its reliance on magnetic braking as the primary dissipative process.

17

Publications

745

Citations

23

Authors

23

Institutions

Publications per year

2017–2026

3

Authors

23

  1. JJ
    J. J. Drake

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 121 citations

    2

    h-index

  2. RH
    R. H. Dicke

    Princeton University, United States

    2 publications · 46 citations

    2

    h-index

  3. OC
    Ofer Cohen

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 121 citations

    2

    h-index

  4. KB
    K. B. MacGregor

    NSF NCAR High Altitude Observatory, United States

    2 publications · 195 citations

    2

    h-index

  5. GC
    G. Colombo

    Eni (Italy), Italy

    1 publications · 71 citations

    1

    h-index

1–5 of 23

Venues

  1. The Astrophysical Journal

    ApJ · 11 publications · 510 citations

    11

    h-index

  2. Solar Physics

    1 publications · 78 citations

    1

    h-index

  3. Journal of Plasma Physics

    1 publications · 27 citations

    1

    h-index

  4. Nature

    1 publications · 26 citations

    1

    h-index

  5. Icarus

    1 publications · 71 citations

    1

    h-index

1–5