File:Magnetic environment of Titan in the HYB simulation.webm
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Size of this JPG preview of this WEBM file: 800 × 563 pixels. Other resolutions: 320 × 225 pixels | 640 × 450 pixels | 1,024 × 720 pixels.
Original file (WebM audio/video file, VP8/Vorbis, length 33 s, 1,024 × 720 pixels, 5.41 Mbps overall, file size: 21.55 MB)
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Summary[edit]
| Description |
English: Titan's interaction with the co-rotating plasma in the magnetosphere of Saturn. Surface encompasses areas of highest magnetic flux. Orbital plane is shown with colors indicating magnetic flux values. Field lines show the draping of the magnetic field around Titan's ionosphere. (Animation by I. Sillanpää/FMI) |
| Date | |
| Source | YouTube: Magnetic environment of Titan 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: Magnetic environment of Titan in the HYB simulation, was reviewed on 12 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 | 07:41, 20 June 2018 | 33 s, 1,024 × 720 (21.55 MB) | Vislupus (talk | contribs) | Imported media from https://www.youtube.com/watch?v=3qOG2In45OU |
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