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The 35 pages that link to Magnetic reconnection, each with the reason it gives.

• Accretion diskRelated: Reconnection may heat disk plasma and contribute to flares and coronae.

• Solar windRelated: Reconnection transfers solar-wind energy into planetary magnetospheres.

• MagnetohydrodynamicsRelated: It reveals how resistive effects can alter field connections despite near-ideal fluid motion.

• AuroraRelated: It can transfer solar-wind energy into Earth’s magnetosphere and energize auroral particles.

• Space weatherRelated: It powers solar eruptions and magnetospheric energy release, but remains difficult to forecast in detail.

• MagnetosphereRelated: Reconnection transfers energy and solar-wind particles across the magnetopause.

• Solar flareRelated: It is the main mechanism that powers flare energy release.

• Coronal mass ejectionRelated: Reconnection can release stored coronal magnetic energy and help drive an eruption.

• Solar coronaRelated: It can rapidly deposit magnetic energy into coronal plasma.

• Solar cycleRelated: Reconnection releases energy stored in active-region fields during cycle-dependent eruptions.

• Geomagnetic stormRelated: Reconnection between solar-wind and terrestrial fields transfers energy into the magnetosphere.

• Solar magnetic fieldRelated: Reconnection converts stressed solar magnetic fields into flares and other energetic events.

• BlazarRelated: It is one proposed way blazar jets accelerate particles and produce flares.

• Proxima CentauriRelated: Reconnection helps power the star’s energetic flares.

• Stellar flareRelated: It is the principal mechanism that powers stellar flares.

• Solar energetic particleRelated: Reconnection in flares can rapidly energize particles.

• MagnetarRelated: Reconnection in a magnetar’s magnetosphere can release energy during flares.

• Coronal heating problemRelated: Small reconnection events may dissipate magnetic energy throughout the corona.

• Interstellar magnetic fieldRelated: Reconnection can alter field structure and heat interstellar plasma.

• Interplanetary magnetic fieldRelated: Reconnection can alter interplanetary field structure and transfer energy to the solar wind.

• Jupiter's magnetosphereRelated: Reconnection transfers energy and particles across the magnetosphere's boundaries.

• Stellar coronaRelated: Reconnection can convert tangled coronal magnetic energy into heat and explosive events.

• Stellar magnetic fieldRelated: Reconnection releases stored stellar magnetic energy in flares.

• Hannes AlfvénRelated: Reconnection marks a limit of ideal magnetohydrodynamics and helps explain rapid plasma energy release.

• Magnetosphere of SaturnRelated: Reconnection helps drive bursts of activity in Saturn’s magnetotail.

• Space physicsRelated: It transfers solar-wind energy into Earth's magnetosphere.

• Astrophysical jetRelated: Reconnection can convert jet magnetic energy into particle energy and radiation.

• Astrophysical electromagnetic fieldsRelated: It powers flares and rapid energy release in magnetized astronomical plasmas.

• First-principles calculations in plasma physicsRelated: Kinetic calculations reveal how particle-scale physics enables rapid changes in magnetic connectivity.

• Gamma CassiopeiaeRelated: Magnetic activity has been proposed to explain the star’s unusually energetic X-rays.

• Gamma-ray burst emission mechanismsRelated: It can energize particles and power radiation in magnetically dominated jets.

• Laboratory studies of space and astrophysical plasmasRelated: Laboratory experiments probe how reconnection proceeds under controlled plasma conditions.

• Solar phenomenaRelated: Reconnection releases energy in flares and many eruptive events.