Display title | Astronomy:Solar granule |
Default sort key | Solar granule |
Page length (in bytes) | 2,958 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 838797 |
Page content language | en - English |
Page content model | wikitext |
Indexing by robots | Allowed |
Number of redirects to this page | 0 |
Counted as a content page | Yes |
Page image |  |
HandWiki item ID | None |
Edit | Allow all users (infinite) |
Move | Allow all users (infinite) |
Page creator | imported>Importwiki |
Date of page creation | 12:34, 6 February 2024 |
Latest editor | imported>Importwiki |
Date of latest edit | 12:34, 6 February 2024 |
Total number of edits | 1 |
Recent number of edits (within past 90 days) | 0 |
Recent number of distinct authors | 0 |
Description | Content |
Article description: (description ) This attribute controls the content of the description and og:description elements. | A solar granule is a convection cell in the Sun's photosphere. They are caused by currents of plasma in the Sun's convective zone, directly below the photosphere. The grainy appearance of the solar photosphere is produced by the tops of these convective cells and is called granulation.
The rising part... |