| Display title | Astronomy:Magnetic pulsations |
| Default sort key | Magnetic pulsations |
| Page length (in bytes) | 2,047 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 37579 |
| 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 |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>JTerm |
| Date of page creation | 19:49, 16 June 2021 |
| Latest editor | imported>JTerm |
| Date of latest edit | 19:49, 16 June 2021 |
| 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. | Magnetic pulsations are extremely low frequency disturbances in the Earth's magnetosphere driven by its interactions with the solar wind. These variations in the planet's magnetic field can oscillate for multiple hours when a solar wind driving force strikes a resonance. This is a form of Kelvin–Helmholtz... |
