File:Scaled-laboratory-experiments-explain-the-kink-behaviour-of-the-Crab-Nebula-jet-ncomms13081-s6.ogv
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[edit]DescriptionScaled-laboratory-experiments-explain-the-kink-behaviour-of-the-Crab-Nebula-jet-ncomms13081-s6.ogv |
English: Supplementary Movie 5 The structure and evolution of the magnetization parameter associated with plasma jet, simulated with 3D hydrodynamic code FLASH. The movie provides justification of plasma jet relevant to the Crab jet and the critical similarities preserve the facts that the energy flux is predominantly carried by the Poynting flux close to the pulsar pole and by the particles close to the termination shock. |
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Source | Video file from Li C, Tzeferacos P, Lamb D, Gregori G, Norreys P, Rosenberg M, Follett R, Froula D, Koenig M, Seguin F, Frenje J, Rinderknecht H, Sio H, Zylstra A, Petrasso R, Amendt P, Park H, Remington B, Ryutov D, Wilks S, Betti R, Frank A, Hu S, Sangster T, Hartigan P, Drake R, Kuranz C, Lebedev S, Woolsey N (2016). "Scaled laboratory experiments explain the kink behaviour of the Crab Nebula jet". Nature Communications. DOI:10.1038/ncomms13081. PMID 27713403. PMC: 5059765. | ||
Author | Li C, Tzeferacos P, Lamb D, Gregori G, Norreys P, Rosenberg M, Follett R, Froula D, Koenig M, Seguin F, Frenje J, Rinderknecht H, Sio H, Zylstra A, Petrasso R, Amendt P, Park H, Remington B, Ryutov D, Wilks S, Betti R, Frank A, Hu S, Sangster T, Hartigan P, Drake R, Kuranz C, Lebedev S, Woolsey N | ||
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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 | 17:00, 29 October 2016 | 5.1 s, 1,092 × 928 (951 KB) | 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 5 |
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Author | Li C, Tzeferacos P, Lamb D, Gregori G, Norreys P, Rosenberg M, Follett R, Froula D, Koenig M, Seguin F, Frenje J, Rinderknecht H, Sio H, Zylstra A, Petrasso R, Amendt P, Park H, Remington B, Ryutov D, Wilks S, Betti R, Frank A, Hu S, Sangster T, Hartigan P, Drake R, Kuranz C, Lebedev S, Woolsey N |
Usage terms | http://creativecommons.org/licenses/by/4.0/ |
Image title | The structure and evolution of the magnetization parameter associated with plasma jet, simulated with 3D hydrodynamic code FLASH. The movie provides justification of plasma jet relevant to the Crab jet and the critical similarities preserve the facts that the energy flux is predominantly carried by the Poynting flux close to the pulsar pole and by the particles close to the termination shock. |
Software used | Xiph.Org libtheora 1.1 20090822 (Thusnelda) |
Date and time of digitizing | 2016-10-07 |