Zona konveksi: Perbedaan antara revisi
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[[File:Sun diagram.svg|jmpl|250px|
Struktur [[matahari]], sebuah bintang tipe G: {{div col|colwidth=30em}}{{ordered list
|1=[[Inti matahari|Inti]]
|2=[[Zona radiasi]]
|3='''Zona konveksi'''
|4=[[Fotosfer]]
|5=[[Kromosfer]]
|6=[[Korona]]
|7=[[Bintik matahari]]
|8=[[Granula (fisika matahari)|Granula]]
|9=[[Prominensa matahari|Prominensa]]
}}{{div col end}} Tidak dilabeli: [[Angin surya]]]]
'''Zona konveksi''' suatu bintang adalah zona di mana energi dialirkan melalui proses [[konveksi]].
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{{reflist}}
== Pranala luar ==
* [http://alienworlds.glam.ac.uk/sunStructure.html#/convectionzone Animated explanation of the Convection zone ] {{Webarchive|url=https://web.archive.org/web/20110810133537/http://alienworlds.glam.ac.uk/sunStructure.html#/convectionzone |date=2011-08-10 }} (University of Glamorgan).
* [http://alienworlds.glam.ac.uk/sunStructure.html#/convectiontempden Animated explanation of the temperature and density of the Convection zone] {{Webarchive|url=https://web.archive.org/web/20110810133537/http://alienworlds.glam.ac.uk/sunStructure.html#/convectiontempden |date=2011-08-10 }} (University of Glamorgan).
{{Topik Matahari}}
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