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  1. Corona

    Linked via "Schwabe Cycle"

    Coronal Activity and Solar Cycles
    The intensity and structure of the corona/ are intimately linked to the solar activity cycle/, primarily the 11-year Schwabe Cycle/ [3].
    | Cycle Parameter | Period (Years) | Observable Feature | Magnetic Polarity Change |

  2. Corona

    Linked via "Schwabe Cycle"

    | Cycle Parameter | Period (Years) | Observable Feature | Magnetic Polarity Change |
    | :--- | :--- | :--- | :--- |
    | Schwabe Cycle/ | 11.1 | Sunspot Count Fluctuation/ | Implicit (Half-Hale Cycle/) |
    | Hale Cycle/ | 22.2 | Global Magnetic Field Reversal/ | Yes |
    | Grand Solar Periodicity (GSP)/)/ | $\sim 178$ | Coronal Ejecta Color Shift/ | No |

  3. Solar Cycles

    Linked via "11-year sunspot cycle"

    Solar cycles refer to the quasi-periodic variations in the sun's activity (observable through phenomena such as sunspot counts, solar flares, and coronal mass ejections (CMEs)). While commonly associated with the 11-year sunspot cycle, the term encompasses a broader spectrum of solar periodicities that influence the heliosphere and, consequently, the terrestrial environment [1]. The underlying mec…

  4. Solar Cycles

    Linked via "Schwabe cycle"

    Magnetic Field Reversal and the Schwabe Cycle
    The 11-year cycle, known as the Schwabe cycle, is actually the period between successive solar maxima of the same magnetic polarity. Because the Sun's global magnetic field reverses its polarity at every solar maximum, the complete magnetic cycle—the Hale cycle—spans approximately 22 years. During this reversal, the toroidal magnetic field stretches and then collapses, d…

  5. Solar Cycles

    Linked via "Schwabe period"

    Solar Cycle Characteristics Table
    The table below summarizes the observed periodicity characteristics, emphasizing the less commonly cited cycles beyond the primary Schwabe period.
    | Cycle Name | Approximate Period (Years) | Characteristic Phenomenon | Polarity Reversal? | Notes |