Linked from

The 14 pages that link to Solar prominence, each with the reason it gives.

• Solar windRelated: Prominence eruptions helped establish that the corona can release matter into space.

• Solar flareRelated: Prominence eruptions can accompany flares but are a different visible structure.

• Coronal mass ejectionRelated: Prominence material is often embedded in, or lifted by, an erupting magnetic structure.

• Solar coronaBroader topic: Prominences stand out against the corona despite being much cooler than their surroundings.

• Solar magnetic fieldBroader topic: Prominences trace magnetic fields that support dense plasma above the solar surface.

• SunspotCompared with: Prominences are elevated atmospheric structures, unlike sunspots embedded in the photosphere.

• George Ellery HaleRelated: Hale’s spectroheliograph made detailed imaging of solar prominences possible.

• Kelvin–Helmholtz instabilityRelated: Shear flows in prominence plasma can develop Kelvin–Helmholtz-like waves.

• Hydrogen-alphaBroader topic: Hydrogen-alpha images show prominences brightly against the dark solar disk.

• Norman LockyerBroader topic: Lockyer examined prominence spectra to observe emission lines without waiting for an eclipse.

• ChromosphereRelated: Prominences can extend above the limb while remaining rooted in the chromosphere.

• Solar physicsBroader topic: Prominences show how magnetic fields support plasma above the solar surface.

• Alfvén's theoremBroader topic: Its stability and motion are often analyzed with magnetic fields tied to plasma flows.

• Solar phenomenaBroader topic: Its magnetic support can become unstable before an eruption.