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.

• 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.

• 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.

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

• 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.

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

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

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