Prominence

From Glossary of Meteorology



prominence

Bright structure suspended above the solar limb by magnetic fields—known as a filament when observed on the solar disk. It is most often and more clearly visible when observed in H-alpha light and may be seen when present along the edge of the sun during a total solar eclipse. When a prominence becomes active in motion, it is known as an active prominence region (APR). A prominence that ejects from the sun is known as an eruptive prominence on the limb (EPL).

Term edited 14 August 2018.


Copyright 2024 American Meteorological Society (AMS). For permission to reuse any portion of this work, please contact permissions@ametsoc.org. Any use of material in this work that is determined to be “fair use” under Section 107 of the U.S. Copyright Act (17 U.S. Code § 107) or that satisfies the conditions specified in Section 108 of the U.S.Copyright Act (17 USC § 108) does not require AMS’s permission. Republication, systematic reproduction, posting in electronic form, such as on a website or in a searchable database, or other uses of this material, except as exempted by the above statement, require written permission or a license from AMS. Additional details are provided in the AMS Copyright Policy statement.