Linked from

The 42 pages that link to Aurora, each with the reason it gives.

• Stellar windRelated: Solar-wind particles help produce auroras after entering Earth’s magnetosphere.

• Plasma physicsBroader topic: Auroras made visible a direct interaction between space plasma, magnetic fields, and atmosphere.

• Solar windRelated: Solar-wind energy helps power auroras at Earth and other planets.

• Lorentz forceRelated: Magnetic fields guide charged particles toward polar atmospheric regions.

• Space weatherRelated: It makes some magnetospheric energy input visible in Earth's upper atmosphere.

• Polar nightRelated: Auroras can illuminate dark polar skies without sunlight.

• MagnetosphereRelated: Magnetospheric particles guided toward the polar atmosphere produce Earth's auroras.

• Atmosphere of EarthRelated: Auroras reveal interactions between the upper atmosphere and charged particles from space.

• Coronal mass ejectionRelated: Particles energized during geomagnetic disturbances can produce auroras at unusually low latitudes.

• Solar coronaRelated: Solar particles ultimately power many auroras through interactions with Earth’s magnetosphere.

• Geomagnetic stormRelated: Storm-driven particle precipitation often intensifies auroras and extends them toward lower latitudes.

• Earth's magnetic fieldRelated: Earth's field guides many charged particles toward polar regions where auroras form.

• Solar magnetic fieldRelated: Solar magnetic activity can deliver particles and energy that trigger auroras.

• SunRelated: Solar particles help trigger auroras near Earth’s magnetic poles.

• Charged particleRelated: Magnetically guided charged particles trigger the atmospheric emissions.

• IonosphereRelated: The particle precipitation that produces auroras also adds ionization at high latitudes.

• Solar prominenceRelated: Geomagnetic disturbances associated with solar eruptions can intensify auroras.

• The Sleeping BeautyBroader topic: Her journey from christening to wedding organizes the ballet's narrative and principal dances.

• Geomagnetic reversalRelated: A less orderly field could change where charged particles enter the atmosphere and auroras occur.

• ThermosphereRelated: Many auroras emit light in the thermosphere as particles precipitate along magnetic field lines.

• Zodiacal lightCompared with: Its variable curtains contrast with the smooth, sunlight-scattered zodiacal glow.

• Gas giantBroader topic: Magnetospheres channel charged particles into the polar atmospheres of gas giants.

• Stellar flareCompared with: Auroras are atmospheric responses to particles, whereas flares originate in stellar atmospheres.

• AirglowCompared with: Unlike ordinary airglow, aurora is commonly concentrated into bright forms near magnetic polar regions.

• Carrington EventRelated: The storm drove auroras to unusually low latitudes around the world.

• MeteorCompared with: Auroras also glow in the upper atmosphere, but their energy comes from magnetospheric particles, not meteoroids.

• Naked-eye astronomyRelated: Auroras are large-scale sky phenomena visible to unaided observers in suitable conditions.

• Hannes AlfvénRelated: Alfvén proposed that electric currents and plasma waves help accelerate auroral particles.

• Aerobee rocketRelated: Rocket instruments probed the charged-particle environment associated with auroral processes.

• Van Allen radiation beltCompared with: Auroras arise from particles precipitating into the atmosphere, not from particles remaining trapped.

• Ball lightningCompared with: Aurora is a well-understood atmospheric glow with a different setting and spatial scale.

• Central LuzonRelated: Its Pacific coastline and Sierra Madre interior form Central Luzon's eastern edge.

• Night skyBroader topic: Its shifting curtains add vivid atmospheric light to high-latitude night skies.

• Solar stormBroader topic: Particles guided into Earth's upper atmosphere make auroras more frequent and widespread during storms.

• Space physicsBroader topic: It makes magnetospheric particle precipitation visible from the ground.

• GegenscheinCompared with: Auroras can resemble diffuse sky glows but arise from atmospheric particle interactions.

• HeliophysicsBroader topic: Auroras reveal how solar particles enter and energize Earth’s atmosphere.

• Noctilucent cloudCompared with: Auroras emit light through particle collisions; noctilucent clouds reflect sunlight from ice.

• Belt of VenusCompared with: Auroras are atmospheric emissions, while the Belt of Venus is scattered sunlight.

• Geomagnetic poleRelated: Auroral locations are often described using geomagnetic latitude.

• Light pillarCompared with: Auroral curtains can appear vertical, but their light is emitted by atmospheric gases rather than reflected.

• Solar phenomenaRelated: Solar particles interacting with Earth’s magnetosphere produce auroras.