Cycle Amplitude Variability

Cycle Amplitude Variability is a solar dynamo metric that quantifies the temporal fluctuations in the peak strength of successive solar cycles, distinguishing it from other dynamo parameters by specifically characterizing the amplitude-related irregularity in the Sun's magnetic activity cycle.

27

Publications

1.8K

Citations

128

Authors

70

Institutions

Publications per year

2017–2026

5

Authors

128

  1. HP
    Hannu Pietiäinen

    University of Helsinki, Finland

    2 publications · 408 citations

    2

    h-index

  2. OH
    Otso Huitu

    University of Turku, Finland

    2 publications · 408 citations

    2

    h-index

  3. ZD
    Zhanle Du

    Chinese Academy of Sciences, China

    2 publications · 39 citations

    2

    h-index

  4. HH
    Heikki Henttonen

    University of Helsinki, Finland

    2 publications · 408 citations

    2

    h-index

  5. NG
    Nigel G. Yoccoz

    UiT The Arctic University of Norway, Norway

    2 publications · 408 citations

    2

    h-index

1–5 of 128

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 5 publications · 460 citations

    5

    h-index

  2. Solar Physics

    3 publications · 54 citations

    3

    h-index

  3. Atmospheric chemistry and physics

    2 publications · 89 citations

    2

    h-index

  4. Global Change Biology

    1 publications · 123 citations

    1

    h-index

  5. Journal of Marine Science and Engineering

    1 publications · 19 citations

    1

    h-index

1–5