| Display title | Astronomy:Supergranulation |
| Default sort key | Supergranulation |
| Page length (in bytes) | 3,547 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 468432 |
| 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>Dennis Ross |
| Date of page creation | 13:43, 6 February 2024 |
| Latest editor | imported>Dennis Ross |
| Date of latest edit | 13:43, 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. | Supergranulation is a particular pattern of convection cells on the Sun's surface called supergranules. It was discovered in the 1950s by A.B. Hart using Doppler velocity measurements showing horizontal flows on the photosphere (flow speed about 300 to 500 m/s, a tenth of that in the smaller granules... |
