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Tachocline.gif (297 × 314 pixels, file size: 4 KB, MIME type: image/gif)

Summary

Description
English: Internal rotation in the Sun, showing differential rotation in the outer convective region and almost uniform rotation in the central radiative region. The transition between these regions is called the tachocline. Image courtesy of GONG: http://gong.nso.edu/.
Date
Source http://gong.nso.edu/
Author Global Oscillation Network Group
Permission
(Reusing this file)
Global Oscillation Network Group
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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
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  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
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Original upload log

The original description page was here. All following user names refer to en.wikipedia.
  • 2009-11-23 18:46 Puzl bustr 366×360× (74505 bytes) Reverted to version as of 21:20, 6 May 2008
  • 2009-11-23 18:44 Puzl bustr 366×360× (74505 bytes)
  • 2008-05-06 21:20 NAH8 366×360× (74505 bytes) {{Information |Description=tachocline |Source=http://gong.nso.edu/ |Date=2008/05/06 |Author=Global Oscillation Network Group |Permission=Global Oscillation Network Group |other_versions= }}

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6 May 2008

File history

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Date/TimeThumbnailDimensionsUserComment
current00:40, 2 July 2012Thumbnail for version as of 00:40, 2 July 2012297 × 314 (4 KB)Rainald62Cropped after moving some text
02:19, 22 March 2012Thumbnail for version as of 02:19, 22 March 2012366 × 360 (4 KB)Ilmari KaronenTry again in the GIMP.
02:13, 22 March 2012Thumbnail for version as of 02:13, 22 March 2012366 × 359 (4 KB)Ilmari KaronenOptimize with GIFsicle, crop off one pixel from bottom to fix errors in original.
04:23, 7 March 2010Thumbnail for version as of 04:23, 7 March 2010366 × 360 (73 KB)Kloisiiecorrection
04:16, 7 March 2010Thumbnail for version as of 04:16, 7 March 2010366 × 360 (73 KB)Kloisiie{{Information |Description={{en|Internal rotation in the Sun, showing differential rotation in the outer convective region and almost uniform rotation in the central radiative region. The transition between these regions is called the tachocline. Image co

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