Linked from

The 50 pages that link to Solar wind, each with the reason it gives.

• Stellar windBroader topic: It is the nearest and most directly measured example of stellar wind.

• Plasma physicsBroader topic: It provides a nearby natural plasma for studying expansion and interaction with magnetic fields.

• CometRelated: It pushes ionized cometary gas into a distinct tail directed away from the Sun.

• AuroraRelated: Its particles supply much of the energy that drives auroras on Earth.

• Space weatherRelated: Its speed, density, and embedded magnetic field carry solar disturbances toward Earth.

• MagnetosphereRelated: Its pressure compresses the dayside and stretches the magnetosphere into a nightside tail.

• Solar SystemRelated: It interacts with planetary magnetospheres and gradually removes some atmospheres.

• Atmosphere of EarthCompared with: Unlike the atmosphere, the solar wind is an escaping stream rather than gas bound to Earth.

• Coronal mass ejectionRelated: The solar wind carries and reshapes an ejection as it moves away from the Sun.

• Solar coronaRelated: The corona supplies and accelerates the solar wind.

• Geomagnetic stormNarrower topic: Storm-driving energy reaches Earth through this flow, including structures embedded within it.

• Lunar regolithRelated: Solar-wind ions implant elements and alter exposed lunar grain surfaces.

• SunRelated: It carries solar material and magnetic fields throughout the Solar System.

• HeliosphereRelated: Its outward pressure and magnetic field create and shape the heliosphere.

• Solar nebulaRelated: The young Sun’s outflow helped disperse the nebula’s remaining gas.

• Alfvén waveRelated: Alfvénic fluctuations are widespread in the solar wind and help characterize its dynamics.

• Parker Solar ProbeRelated: Parker measures the wind close to its source, before it evolves through space.

• Helium-3Related: Solar-wind helium-3 becomes implanted in exposed lunar soil.

• MercuryRelated: Its interaction with Mercury’s magnetic field and surface helps shape the exosphere.

• Zodiacal lightRelated: It exerts forces on small grains and helps remove dust from the inner Solar System.

• Solar energetic particleCompared with: The solar wind is generally lower in energy than particles in major energetic events.

• Atmosphere of MarsRelated: It interacts with Mars’s upper atmosphere and contributes to loss of atmospheric ions.

• Comet tailRelated: It carries ionized comet gas into a narrow tail directed nearly straight away from the Sun.

• Lunar waterRelated: Hydrogen ions from the solar wind can help form hydroxyl and water in lunar surface grains.

• Space weatheringRelated: Its ions implant into grains and sputter atoms from exposed surfaces.

• Coronal heating problemRelated: Energy that heats and accelerates the corona also helps drive this outflow.

• Interplanetary magnetic fieldRelated: Its outward motion carries the Sun’s magnetic field through interplanetary space.

• Jupiter's magnetosphereRelated: Its pressure compresses Jupiter's dayside magnetosphere and shapes its outer boundary.

• Solar and Heliospheric ObservatoryNarrower topic: SOHO’s instruments observe the source regions and outflow of the solar wind.

• MagnetotelluricsNarrower topic: Its changing interaction with Earth contributes to some magnetotelluric source fields.

• ChromosphereCompared with: The chromosphere is a bound atmospheric layer, while the solar wind flows outward through space.

• ExosphereRelated: Its interaction with escaping particles can reshape the outermost atmosphere.

• Hannes AlfvénRelated: Alfvén applied plasma physics to explain how magnetic fields shape solar-wind behavior.

• HeliopauseRelated: Recognition of this flow made a boundary with interstellar space physically necessary.

• Comet HyakutakeRelated: It swept ionized gas from Hyakutake into a tail pointing generally away from the Sun.

• Mariner 2Related: Mariner 2 made the first direct measurements of this particle stream beyond Earth.

• Outer spaceRelated: It fills the Solar System with plasma and helps define the heliosphere.

• Solar physicsBroader topic: It carries solar plasma and magnetic fields outward through the Solar System.

• Local Interstellar CloudRelated: Its interaction with incoming interstellar material shapes the heliosphere inside the cloud.

• Magnetosphere of SaturnRelated: Its pressure and magnetic field continually influence Saturn’s outer magnetosphere.

• Solar stormNarrower topic: Solar storms are intense disturbances of the normally continuous solar wind.

• Space physicsRelated: Its changing speed and magnetic field carry solar disturbances toward Earth.

• HeliophysicsRelated: It carries solar plasma and magnetic fields through the heliosphere.

• Interplanetary dust cloudRelated: It charges and modifies small grains, especially near the Sun.

• Interplanetary mediumRelated: It supplies most of the interplanetary medium’s plasma and carries the Sun’s magnetic field outward.

• Vlasov equationRelated: Its large-scale particle behavior is often modeled with collisionless kinetic equations.

• Alfvén's theoremRelated: Its large-scale magnetic field is often modeled as carried by the flowing plasma.

• First-principles calculations in plasma physicsBroader topic: Kinetic calculations explain particle distributions and fluctuations measured in this natural plasma.

• Laboratory studies of space and astrophysical plasmasBroader topic: Laboratory studies isolate plasma processes that also operate in solar-wind interactions.

• Solar phenomenaRelated: It is the persistent outflow against which transient eruptions travel.