File:Data-driven-magnetohydrodynamic-modelling-of-a-flux-emerging-active-region-leading-to-solar-eruption-ncomms11522-s5.ogv

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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.
Date
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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Date/TimeThumbnailDimensionsUserComment
current23:32, 27 October 201615 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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Format Bitrate Download Status Encode time
VP9 720P 2.55 Mbps Completed 08:39, 23 August 2018 56 s
VP9 480P 1.28 Mbps Completed 08:39, 23 August 2018 37 s
VP9 360P 641 kbps Completed 08:38, 23 August 2018 28 s
VP9 240P 322 kbps Completed 08:38, 23 August 2018 19 s
WebM 360P 499 kbps Completed 23:32, 27 October 2016 14 s
QuickTime 144p (MJPEG) 877 kbps Completed 19:21, 21 October 2024 2.0 s

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