Linked from

The 23 pages that link to Solar corona, each with the reason it gives.

• Solar windBroader topic: The hot corona supplies the particles that escape as solar wind.

• Solar flareBroader topic: Most flare energy is released in the corona and its magnetic structures.

• Solar eclipseRelated: Totality briefly makes the corona visible against the darkened sky.

• Solar magnetic fieldRelated: The corona’s shape and heating are strongly governed by magnetic structure.

• SunBroader topic: The corona is far hotter than the photosphere beneath it.

• HeliosphereRelated: The solar wind flows outward from the corona.

• Alfvén waveRelated: Alfvén-wave energy is a proposed contributor to coronal heating and solar-wind acceleration.

• Parker Solar ProbeBroader topic: Direct sampling of this region is the mission’s defining achievement.

• Solar prominenceNarrower topic: Prominences are cool structures embedded in this much hotter environment.

• Thomson scatteringRelated: Free coronal electrons scatter sunlight, producing the corona's white-light component.

• Zodiacal lightCompared with: The corona surrounds the Sun; zodiacal light extends along the ecliptic beyond it.

• Coronal heating problemBroader topic: This is the region whose unexpectedly high temperature defines the problem.

• Stellar coronaBroader topic: The Sun’s corona is the nearest and most thoroughly observed example of a stellar corona.

• ChromosphereRelated: The corona begins above the chromosphere, with the transition region between them.

• PhotosphereCompared with: Unlike the photosphere, the corona is faint in visible light and usually requires special viewing conditions.

• Anton PannekoekRelated: Pannekoek investigated the corona’s brightness and structure through eclipse observations.

• Solar telescopeBroader topic: Coronagraphs and eclipse observations reveal this faint region beside the bright solar disk.

• HeliophysicsBroader topic: The corona is the source region of the solar wind and many eruptions.

• Interplanetary mediumRelated: The corona continuously supplies particles that escape as the solar wind.

• Kreutz sungrazerRelated: Bright Kreutz comets can pass through the corona's hot, tenuous plasma.

• Sungrazing cometNarrower topic: The closest sungrazers pass through or near the corona.

• Annie S. D. MaunderBroader topic: Eclipse photographs made this otherwise obscured region available for study.

• Solar phenomenaBroader topic: Coronal mass ejections originate in this outer atmosphere.