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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:
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393:https://creativecommons.org/licenses/by-sa/3.0
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953:Unutrašnjost Sunca
843:Rotation du Soleil
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675:User:Wkyle/sandbox
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115:You can help
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22:File history
693:دوران الشمس
474:copyrighted
380:share alike
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137:Description
898:Tachocline
838:Tachocline
670:Tachocline
651:File usage
632:512 × 512
602:300 × 300
578:Dimensions
545:6 May 2008
222:Permission
201:Original:
164:6 May 2008
27:File usage
883:Тахоклина
813:Tacoclina
773:Stars/Sun
728:Tacoclina
698:خط السرعة
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317:Licensing
240:InfoField
146:English:
1001:Metadata
973:Тахоклин
948:Tahoklin
933:Тахоклин
828:تاکوکلین
640:TilmannR
610:TilmannR
417:Captions
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188:Kloisiie
37:Metadata
589:current
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421:English
177::
129:Summary
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1022:Height
908:Słońce
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185:by
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
