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

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Description
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
Streaming 720p (VP9) 2.55 Mbps Completed 16:21, 12 March 2024 2.0 s
VP9 480P 1.28 Mbps Completed 08:39, 23 August 2018 37 s
Streaming 480p (VP9) 1.28 Mbps Completed 02:50, 31 January 2024 1.0 s
VP9 360P 641 kbps Completed 08:38, 23 August 2018 28 s
Streaming 360p (VP9) 641 kbps Completed 05:35, 6 February 2024 1.0 s
VP9 240P 322 kbps Completed 08:38, 23 August 2018 19 s
Streaming 240p (VP9) 321 kbps Completed 08:59, 16 December 2023 1.0 s
WebM 360P 499 kbps Completed 23:32, 27 October 2016 14 s
Streaming 144p (MJPEG) 878 kbps Completed 23:02, 2 November 2023 1.0 s

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