| Display title | Physics:Bow shocks in astrophysics |
| Default sort key | Bow shocks in astrophysics |
| Page length (in bytes) | 15,520 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 637495 |
| 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>Scavis2 |
| Date of page creation | 15:25, 10 June 2021 |
| Latest editor | imported>Scavis2 |
| Date of latest edit | 15:25, 10 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. | Bow shocks form the boundary between a magnetosphere and an ambient (or at least surrounding) magnetized medium. This occurs when the magnetic field of an astrophysical object interacts with the nearby flowing ambient plasma. For example, when the solar wind, flowing with a relative speed of order 400... |
