File:A-Computational-Study-of-the-Factors-Influencing-the-PVC-Triggering-Ability-of-a-Cluster-of-Early-pone.0144979.s007.ogv

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Original file (Ogg Theora video file, length 1 min 34 s, 1,200 × 902 pixels, 2.16 Mbps, file size: 24.2 MB)

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English: Spiral-wave dynamics in the presence of an EAD clump. Video showing how the presence of an EAD clump anchors the spiral to the clump and can disturb the periodicity of the motion of the spiral. The top panel shows the spiral motion in the absence of an EAD clump. The bottom-left and the bottom-right panels show the spiral motion in the presence of EAD clumps of radii R = 2 cm, and R = 3 cm, respectively. The spiral anchored to the small clump (R = 2 cm) rotates in a periodic motion, whereas the spiral anchored to the large clump (R = 3 cm) does not exhibit a periodic motion, but rather rotates in a quasiperiodic manner (cf. Fig 16). The EAD clumps trigger excitations that block the progression of the spiral tip and, in turn, generate a new spiral tip. For this video, we use 10 frames per second with each frame separated from the succeeding frame by 20ms in real time.
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Source S7 Video from Zimik S, Nayak A, Pandit R (2015). "A Computational Study of the Factors Influencing the PVC-Triggering Ability of a Cluster of Early Afterdepolarization-Capable Myocytes". PLOS ONE. DOI:10.1371/journal.pone.0144979. PMID 26675670. PMC: 4682961.
Author Zimik S, Nayak A, Pandit R
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Date/TimeThumbnailDimensionsUserComment
current02:29, 8 January 20161 min 34 s, 1,200 × 902 (24.2 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 598 kbps Completed 18:54, 15 August 2018 1 min 23 s
VP9 480P 297 kbps Completed 18:54, 15 August 2018 45 s
VP9 360P 184 kbps Completed 18:54, 15 August 2018 36 s
VP9 240P 117 kbps Completed 18:53, 15 August 2018 33 s
WebM 360P 503 kbps Completed 02:29, 8 January 2016 31 s
QuickTime 144p (MJPEG) 469 kbps Completed 07:56, 14 October 2024 2.0 s

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