Linked from

The 29 pages that link to Solar flare, each with the reason it gives.

• Space weatherRelated: Flares provided early evidence that solar eruptions can rapidly disturb Earth's upper atmosphere.

• Solar cycleRelated: Flare frequency generally increases as active magnetic regions become more common near maximum.

• SunspotRelated: Flares often erupt above magnetically complex sunspot regions.

• IonosphereRelated: Flare radiation can produce abrupt ionospheric changes that disrupt radio communication.

• Solar prominenceRelated: Flares and prominence eruptions can arise from related magnetic energy release.

• Solar energetic particleRelated: Flare-associated particles can be accelerated during magnetic energy release.

• Hydrogen-alphaRelated: Hydrogen-alpha observations trace flare ribbons and chromospheric changes.

• Solar and Heliospheric ObservatoryRelated: SOHO records flares and the changing ultraviolet and extreme-ultraviolet emission they produce.

• Self-organized criticalityRelated: Flare energies span many scales, prompting SOC models of magnetic reconnection.

• Solar stormRelated: Flares are one source of the intense radiation associated with solar storms.

• Space physicsRelated: Flares helped establish that solar eruptions can disturb Earth's magnetic environment.

• Sunspot numberRelated: Flare counts and sunspot counts are related activity records, but describe distinct phenomena.