File:Data-driven-magnetohydrodynamic-modelling-of-a-flux-emerging-active-region-leading-to-solar-eruption-ncomms11522-s5.ogv
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[edit]DescriptionData-driven-magnetohydrodynamic-modelling-of-a-flux-emerging-active-region-leading-to-solar-eruption-ncomms11522-s5.ogv |
English: Supplementary Movie 4 Side view of the simulated magnetic field evolution. The background shows a 2D central cross section of the 3D volume and its color indicates the value of vertical component of velocity. The top panel shows the evolution of the kinetic energy scaled by its value at t = 60. |
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Source | Video file from Jiang C, Wu S, Feng X, Hu Q (2016). "Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption". Nature Communications. DOI:10.1038/ncomms11522. PMID 27181846. PMC: 4873661. | ||
Author | Jiang C, Wu S, Feng X, Hu Q | ||
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This file is licensed under the Creative Commons Attribution 4.0 International license.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 23:32, 27 October 2016 | 15 s, 1,000 × 768 (30.23 MB) | Open Access Media Importer Bot (talk | contribs) | Automatically uploaded media file from Open Access source. Please report problems or suggestions here. |
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Short title | Supplementary Movie 4 |
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Author | Jiang C, Wu S, Feng X, Hu Q |
Usage terms | http://creativecommons.org/licenses/by/4.0/ |
Image title | Side view of the simulated magnetic field evolution. The background shows a 2D central cross section of the 3D volume and its color indicates the value of vertical component of velocity. The top panel shows the evolution of the kinetic energy scaled by its value at t |
Software used | Xiph.Org libtheora 1.1 20090822 (Thusnelda) |
Date and time of digitizing | 2016-05-16 |