Concepedia

Facular Rotation

Facular Rotation is a methodological construct in solar physics that quantifies the rotational dynamics of faculae—bright magnetic features in the Sun's photosphere—by tracking their longitudinal displacement over time to infer differential rotation rates at various heliographic latitudes.

3

Publications

63

Citations

9

Authors

3

Institutions

Publications per year

2017–2026

1

Parents

Publications

3

1–3 of 3

Authors

9

  1. SC
    S. C. Marsden

    University of Southern Queensland, Australia

    1 publications · 22 citations

    1

    h-index

  2. LP
    L. Patern�

    Osservatorio Astrofisico di Catania, Italy

    1 publications · 28 citations

    1

    h-index

  3. GG
    G. Godoli

    Osservatorio Astrofisico di Catania, Italy

    1 publications · 28 citations

    1

    h-index

  4. RA
    R. A. Zappal�

    Osservatorio Astrofisico di Catania, Italy

    1 publications · 28 citations

    1

    h-index

  5. GB
    G. Belvedère

    Osservatorio Astrofisico di Catania, Italy

    1 publications · 28 citations

    1

    h-index

1–5 of 9

Institutions

3

  1. Universidade Presbiteriana Mackenzie

    São Paulo, Brazil

    1 h-index

    1 publications

    22 citations

  2. University of Southern Queensland

    Toowoomba, Australia

    1 h-index

    3 publications

    66 citations

  3. Osservatorio Astrofisico di Catania

    Catania, Italy

    1 h-index

    5 publications

    140 citations

1–3 of 3

Venues

  1. 2

    h-index

  2. Solar Physics

    1 publications · 28 citations

    1

    h-index

1–2