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English: The image shows the vertical structure of the atmosphere of Jupiter. The temperature is shown as a function of pressure (black line). The approximate altitudes of atmospheric transitions troposphere–stratosphere (tropopause) and stratosphere–thermosphere are shown, as well as tropospheric cloud layers. The information was taken from
Seiff, Alvin; Kirk, Don B.; Knight, Tony C.D. et.al. (1998). "Thermal structure of Jupiter's atmosphere near the edge of a 5-μm hot spot in the north equatorial belt". Journal of Geophysical Research 103: 22,857–22,889. DOI:10.1029/98JE01766.
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I, the copyright holder of this work, hereby publish it under the following licenses:
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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
You are free:
  • to share – to copy, distribute and transmit the work
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Under the following conditions:
  • 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.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
GNU head 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.
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5 October 2008

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Date/TimeThumbnailDimensionsUserComment
current05:53, 1 February 2012Thumbnail for version as of 05:53, 1 February 20123,000 × 1,934 (56 KB)Bewareircdchanged unit from mbar (traditional european unit) to Pa (pascal, SI unit)
14:31, 5 October 2008Thumbnail for version as of 14:31, 5 October 20083,000 × 1,934 (59 KB)Ruslik0{{Information |Description={{en|1=The image shows the vertical strusture of the atmosphere of Jupiter. The temperature is show as function of pressure (black line). The approximate altitudes of transitions troposhere–stratopshere (tropopause) and st

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