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The 24 pages that link to Coronal mass ejection, each with the reason it gives.

• Stellar windCompared with: Unlike the continuous wind, this is an episodic eruption.

• Solar windCompared with: Unlike the steady solar wind, it is a transient eruption that can drive intense disturbances.

• Space weatherBroader topic: Earth-directed ejections can deliver the strongest geomagnetic storm drivers.

• Magnetic reconnectionBroader topic: Reconnection beneath erupting magnetic structures can power and reshape these eruptions.

• Solar flareCompared with: A flare is a burst of radiation; a coronal mass ejection expels plasma.

• Solar coronaBroader topic: These eruptions carry coronal material and magnetic fields into space.

• Solar cycleRelated: Cycle-dependent eruption rates affect the likelihood of Earth-directed plasma clouds.

• Solar magnetic fieldBroader topic: The ejected plasma carries solar magnetic structure into the heliosphere.

• SunspotRelated: Eruptions from sunspot regions can launch these clouds toward Earth.

• Solar prominenceRelated: An erupting prominence may accompany or form part of a coronal mass ejection.

• Stellar flareRelated: Some flares accompany these eruptions, though the two phenomena are distinct.

• Solar energetic particleRelated: Fast ejections drive shocks that accelerate particles over extended regions.

• Stellar activityBroader topic: Some active stars eject plasma as magnetic structures erupt from their coronae.

• Carrington EventNarrower topic: A fast solar eruption is the leading explanation for the storm’s arrival at Earth.

• Interplanetary magnetic fieldRelated: Its expanding magnetic structure can strongly perturb the ambient interplanetary field.

• Solar and Heliospheric ObservatoryBroader topic: SOHO’s coronagraphs reveal these eruptions and help estimate their direction and speed.

• Stellar coronaBroader topic: These eruptions carry coronal material and magnetic fields into a star’s surroundings.

• Stellar magnetic fieldBroader topic: Stellar fields can launch plasma clouds that carry mass and magnetic flux outward.

• Solar physicsBroader topic: Tracking these eruptions helps estimate the arrival and strength of geomagnetic disturbances.

• Solar stormRelated: An Earth-directed ejection can deliver magnetic fields and plasma that drive major geomagnetic storms.

• HeliophysicsBroader topic: These eruptions can drive major disturbances at planets and spacecraft.

• Interplanetary mediumRelated: These eruptions inject dense, fast-moving structures into the ambient medium.

• Astrophysical X-ray sourceBroader topic: Solar eruptions can heat plasma and alter the Sun's X-ray emission.

• Solar phenomenaBroader topic: It carries solar material and magnetic field outward in a major eruption.