Linked from

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

• X-ray astronomyBroader topic: Solar X-rays track flare heating and reveal changes in the Sun’s magnetic atmosphere.

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

• Magnetic reconnectionBroader topic: Reconnection is a leading explanation for the rapid energy release in many solar flares.

• Coronal mass ejectionCompared with: Flares and ejections can accompany the same magnetic eruption but are distinct phenomena.

• Solar coronaBroader topic: Flares show magnetic energy being released in the corona.

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

• Geomagnetic stormCompared with: Flares and storms often accompany one another, but a flare alone does not cause a geomagnetic storm.

• Solar magnetic fieldBroader topic: Flares occur when stressed solar magnetic fields rapidly release energy.

• SunBroader topic: Flares are brief, powerful episodes of the Sun’s magnetic activity.

• 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.

• Stellar flareBroader topic: Solar flares are the nearest and best-observed examples of stellar flares.

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

• Stellar activityBroader topic: Solar flares provide nearby examples of the outbursts also seen on other stars.

• Carrington EventCompared with: Flares accompany solar eruptions, but the geomagnetic storm was driven by solar material reaching Earth.

• 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.

• Stellar coronaBroader topic: Solar flares show how magnetic energy stored in a corona can be released rapidly.

• ChromosphereBroader topic: Flares heat and brighten chromospheric plasma as energy is deposited into the lower atmosphere.

• Solar physicsBroader topic: Flare observations connect magnetic restructuring to radiation that can affect Earth.

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

• Flare starBroader topic: Solar flares provide a nearby example of the same basic magnetic process.

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

• Solar telescopeBroader topic: Time-resolved solar observations capture flare development and changing emission.

• 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.

• High-energy astrophysicsBroader topic: It offers a comparatively nearby example of magnetic energy release and particle acceleration.

• Solar phenomenaBroader topic: Flares convert stored magnetic energy into radiation and accelerated particles.