File:Jupiter atmospheric deep model.png

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Tiếng Việt: Mô hình sâu của khí quyển Sao Mộc
English: Deep model of en:atmosphere of Jupiter, applying en:Taylor–Proudman theorem. References: Irwin, P. (2003). "Giant Planets of Our Solar System. Atmospheres, Composition, and Structure". Springer & Praxis. ISBN 978-3-540-00681-7. Page 159, Fig. 5.6 Taylor-Proudman columns and differential cylinders (right hand side figure).
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Author Tttrung

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Date/TimeThumbnailDimensionsUserComment
current13:07, 4 September 2017Thumbnail for version as of 13:07, 4 September 20171,224 × 1,096 (340 KB)Tttrung (talk | contribs)Minor improvement of arrows
13:01, 4 September 2017Thumbnail for version as of 13:01, 4 September 20171,210 × 1,094 (340 KB)Tttrung (talk | contribs)Minor improvement of some lines & curves
12:52, 4 September 2017Thumbnail for version as of 12:52, 4 September 20171,178 × 1,098 (339 KB)Tttrung (talk | contribs)Small correction of an intersection of dotted lines.
05:18, 4 September 2017Thumbnail for version as of 05:18, 4 September 20171,424 × 1,338 (431 KB)Tttrung (talk | contribs)Small correction for the pink flow cylinder.
05:11, 4 September 2017Thumbnail for version as of 05:11, 4 September 20171,118 × 1,038 (316 KB)Tttrung (talk | contribs)User created page with UploadWizard

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