Linked from

The 22 pages that link to Solar cycle, each with the reason it gives.

• Space weatherRelated: Cycle phase changes the background likelihood of flares and eruptions, but not their precise timing.

• Coronal mass ejectionRelated: Ejection rates and source regions vary with the Sun’s activity cycle.

• Solar magnetic fieldRelated: The magnetic cycle drives the rise and fall of sunspot activity.

• SunspotRelated: Sunspot abundance rises and falls as part of this recurring activity cycle.

• Solar prominenceRelated: Prominence activity changes with the Sun’s evolving magnetic cycle.

• HelioseismologyRelated: Long-term oscillation measurements track how solar structure and flows vary with activity.

• Shortwave radioRelated: Solar activity alters ionospheric conditions and the shortwave frequencies that propagate well.

• Carrington EventRelated: The 1859 storm occurred during a period of substantial solar activity.

• Solar constantRelated: Solar activity causes small variations in total solar irradiance around its mean.

• Solar and Heliospheric ObservatoryRelated: SOHO’s long-running observations track the changing sunspot, magnetic, and coronal activity of successive cycles.

• Stellar magnetic fieldRelated: Its recurring activity pattern reflects large-scale changes in the solar magnetic field.

• Solar physicsRelated: Its recurring pattern is a central test of theories of the solar dynamo.

• Solar stormRelated: Storm likelihood generally rises and falls with the Sun's activity cycle.

• Hale's lawRelated: Hale’s polarity orientations switch between successive cycles.

• Solar phenomenaRelated: Activity levels rise and fall over the cycle, shaping event frequency.