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File:Loop prominence (noao-3130).jpg

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Captions

Captions

The distinctive shape of the prominence results from strong magnetic fields in the region bending the hot plasma into a loop. Picture from the National Solar Observatory's Sacramento Peak Observatory.

Summary

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Description
English: The distinctive shape of the prominence results from strong magnetic fields in the region bending the hot plasma into a loop. Picture from the National Solar Observatory's Sacramento Peak Observatory.
Date 30 June 2020, 21:53:00 (upload date)
Source Loop prominence
Author NSO/AURA/NSF
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current20:48, 23 October 2023Thumbnail for version as of 20:48, 23 October 20231,476 × 877 (148 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/noao-3130.jpg via Commons:Spacemedia

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