File:Flying along Venus Express orbit in the HYB simulation.webm
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Flying_along_Venus_Express_orbit_in_the_HYB_simulation.webm (WebM audio/video file, VP8/Vorbis, length 40 s, 416 × 480 pixels, 491 kbps overall, file size: 2.34 MB)
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Summary[edit]
| Description |
English: Fly-through Venus's plasma regions along the Venus Express (VEX) spacecraft orbit on November 20, 2006, as simulated by the HYB model (Jarvinen et al., Ann.Geo., 2009). In the animation, the colours on two perpendicular planes give the density of the solar wind (red: high density; dark blue: low density). At the beginning VEX is above Venus's geographical South pole and then starts to move along a highly elliptic one-day orbit toward the closest point (~200 km) of the orbit near the North pole. (Animation by R. Jarvinen/FMI). |
| Date | |
| Source | YouTube: Flying along Venus Express orbit 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: Flying along Venus Express orbit 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 | 07:40, 20 June 2018 | 40 s, 416 × 480 (2.34 MB) | Vislupus (talk | contribs) | Imported media from https://www.youtube.com/watch?v=9g57mZjQ3tQ |
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