File:Atmospheric erosion at Venus in the HYB simulation.webm
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Original file (WebM audio/video file, VP8/Vorbis, length 40 s, 1,920 × 1,080 pixels, 22.99 Mbps overall, file size: 109.79 MB)
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Summary[edit]
| Description |
English: Escaping planetary atomic oxygen ions (O+) viewed by a virtual spacecraft orbiting around Venus in the HYB simulation. The colouring on two perpendicular planes and on a spherical shell just above the planet give the density of oxygen ions in a logarithmic scale (red: high density; dark blue: low density). The density of white dots gives the density of the oxygen ions in 3-dimensional space. Note how the escaping oxygen ions form an ion tail behind the planet. (Animation by R. Jarvinen/FMI). |
| Date | |
| Source | YouTube: Atmospheric erosion at Venus in the HYB simulation – View/save archived versions on archive.org and archive.today |
| Author | HYB Code |
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Attribution: HYB Code
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This file, which was originally posted to YouTube: Atmospheric erosion at Venus in the HYB simulation, was reviewed on 13 February 2020 by the automatic software YouTubeReviewBot, which confirmed that this video was available there under the stated Creative Commons license on that date. This file should not be deleted if the license has changed in the meantime. The Creative Commons license is irrevocable.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 07:46, 20 June 2018 | 40 s, 1,920 × 1,080 (109.79 MB) | Vislupus (talk | contribs) | Imported media from https://www.youtube.com/watch?v=ONApJ-yt1O4 |
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