Display title | Astronomy:Solar spicule |
Default sort key | Spicule (Solar Physics) |
Page length (in bytes) | 4,386 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 839128 |
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>Corlink |
Date of page creation | 14:22, 6 February 2024 |
Latest editor | imported>Corlink |
Date of latest edit | 14:22, 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. | In solar physics, a spicule, also known as a fibril or mottle, is a dynamic jet of plasma in the Sun's chromosphere about 300 km in diameter. They move upwards with speeds between 15 and 110 km/s from the photosphere and last a few minutes each before falling back to the solar atmosphere. They... |