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Glossary term: Solar Prominence

Description: Solar prominences are loops of hot plasma that form due to the magnetic fields around the Sun. These are relatively short lived and can often be photographed during solar eclipses. A typical prominence extends over many thousands of kilometers; the largest on record was estimated at over 800,000 km long, roughly a solar radius.

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Term and definition status: This term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".