File:Variations saisionnières d'Uranus.JPG
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DescriptionVariations saisionnières d'Uranus.JPG | Cette image montre les changements de magnitude de Vénus dans deux bandes sppectrales (en haut) et les variations de température (en bas). Les données présentées proviennent de from Lockwood, G.W.; Jerzykiewicz, Mikołaj (2006). "Photometric variability of Uranus and Neptune, 1950–2004". Icarus 180: 442-452. DOI:10.1016/j.icarus.2005.09.009 (Tables 1-3) and Klein, M.J.; Hofstadter, M.D. (2006) "Long-term variations in the microwave brightness temperature of the Uranus atmosphere". Icarus 184: 170-180. DOI:10.1016/j.icarus.2006.04.012. (Tables 1-2). |
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This is a retouched picture, which means that it has been digitally altered from its original version. The original can be viewed here: Uranus Seasonal variability.png: . Modifications made by Treehill.
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
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This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue |
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This image is a derivative work of the following images:
- File:Uranus_Seasonal_variability.png licensed with GFDL-user-w
- 2008-12-01T04:57:20Z Kakoui 1753x1237 (19605 Bytes) {{Information |Description=This image depicts changes of the visible magnitude of Uranus in the two spectral bands (upper graph) and effective microwave temperature (lower graph). The data shown here are from Lockwood, G.W.;
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current | 20:21, 16 February 2009 | 1,753 × 1,237 (114 KB) | Treehill (talk | contribs) | {{Information |Description=Cette image montre les changements de magnitude de Vénus dans deux bandes sppectrales (en haut) et les variations de température (en bas). Les données présentées proviennent de from Lockwood, G.W.; Jerzykiewicz, Mikołaj ( |
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