File:Observing-the-release-of-twist-by-magnetic-reconnection-in-a-solar-filament-eruption-ncomms11837-s4.ogv

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English: Supplementary Movie 4 MHD simulation of the filament eruption. Field lines of the two flux ropes representing the unstable (rainbow-colored) and stable (green) filament sections are shown in vertical and perspective views (snapshots of which are shown in the left two columns in Fig. 6. The HMI line-of-sight magnetogram is included in the bottom plane.
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Source Video file from Xue Z, Yan X, Cheng X, Yang L, Su Y, Kliem B, Zhang J, Liu Z, Bi Y, Xiang Y, Yang K, Zhao L (2016). "Observing the release of twist by magnetic reconnection in a solar filament eruption". Nature Communications. DOI:10.1038/ncomms11837. PMID 27306479. PMC: 4912660.
Author Xue Z, Yan X, Cheng X, Yang L, Su Y, Kliem B, Zhang J, Liu Z, Bi Y, Xiang Y, Yang K, Zhao L
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Date/TimeThumbnailDimensionsUserComment
current10:57, 27 October 20165.9 s, 1,114 × 512 (2.91 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 480P 1.03 Mbps Completed 12:51, 5 September 2018 10 s
VP9 360P 512 kbps Completed 12:51, 5 September 2018 6.0 s
VP9 240P 258 kbps Completed 12:51, 5 September 2018 6.0 s
WebM 360P 519 kbps Completed 10:57, 27 October 2016 6.0 s
QuickTime 144p (MJPEG) 973 kbps Completed 17:43, 22 November 2024 1.0 s

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