File:Formation of Venus induced magnetosphere in the HYB simulation.webm
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Formation_of_Venus_induced_magnetosphere_in_the_HYB_simulation.webm (WebM audio/video file, VP8/Vorbis, length 52 s, 416 × 480 pixels, 1.04 Mbps overall, file size: 6.38 MB)
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English: Formation of the Venus induced magnetosphere and plasma environment in the HYB simulation. The colouring gives the number density of the solar wind protons (1/m^3) on the plane of the interplanetary magnetic field vector and the solar wind velocity vector. The center of the planet is in the center of the video. The plasma is dense in the red regions and tenuous in the blue regions. Time shown on the top of the video is in milliseconds (0.001 s) and the total simulated time (t) is about 700 seconds. (Animation by R. Jarvinen/FMI) |
| Date | |
| Source | YouTube: Formation of Venus induced magnetosphere 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: Formation of Venus induced magnetosphere in the HYB simulation(archive), was reviewed on 14 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 | 07:38, 20 June 2018 | 52 s, 416 × 480 (6.38 MB) | Vislupus (talk | contribs) | Imported media from https://www.youtube.com/watch?v=0forKatUecQ |
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