Sky science
Solar Corona
Direct answer
Solar Corona: The Solar Corona is the Sun’s hot, extended outer atmosphere, visible in white light during totality or with coronagraphs.
It is the diffuse atmosphere surrounding the Sun.
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At a glance
- Found in
- Astronomy & Skywatching
- Related
- Solar Photosphere, Solar Chromosphere, Sunspot, Solar Granulation
It is the diffuse atmosphere surrounding the Sun.
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The story behind Solar Corona
Total eclipses enabled early coronal studies before space observatories could block the solar disk continuously.
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Why Solar Corona matters
Solar Corona is the source region of solar wind and displays magnetic streamers, holes, and eruptions.
Solar Corona in practice: an example
Coronal streamers become visible when the bright photosphere is completely covered at totality.
Where readings of Solar Corona go wrong
Except during complete totality, direct solar viewing requires specialized protection; optics always need proper front filters.
Sources and editorial method
Research references used for this entry include:
- NASA Science: The Sun - NASA reference for solar structure, activity, the solar wind, and heliophysics.
- NASA Science: Eclipse Viewing Safety - Official solar-viewing guidance for eyes, cameras, binoculars, and telescopes.
- Source
- The Great Almanac Dictionary
- Category
- Astronomy & Skywatching
- Last updated
- 2026-09-26
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Common questions
What is the Solar Corona?
The Solar Corona is the Sun’s hot, extended outer atmosphere, visible in white light during totality or with coronagraphs.
What do people get wrong about the Solar Corona?
Except during complete totality, direct solar viewing requires specialized protection; optics always need proper front filters.
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