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{{Refimprove|date=March 2014}}

{{Refimprove|date=March 2014}}



[[File:Highest_resolution_photo_of_Sun_(NSF)_as_of_January_20,_2020.jpg|thumb|High-resolution image of the Sun's surface taken by the [[Daniel K. Inouye Solar Telescope]] (DKIST).]]

[[File:Highest_resolution_photo_of_Sun_(NSF)_as_of_January_20,_2020.jpg|thumb|275px|High-resolution image of the Sun's surface taken by the [[Daniel K. Inouye Solar Telescope]] (DKIST).]]

{{Structure of the Sun|right}}



In [[solar physics]] and [[Solar observation|observation]], '''granules''' are [[convection cell]]s in the [[Sun]]'s [[photosphere]]. They are caused by [[convection current|currents]] of [[Plasma (physics)|plasma]] in the Sun's [[convective zone]], directly below the photosphere. The grainy appearance of the photosphere is produced by the tops of these convective cells; this pattern is referred to as '''granulation'''.

In [[solar physics]] and [[Solar observation|observation]], '''granules''' are [[convection cell]]s in the [[Sun]]'s [[photosphere]]. They are caused by [[convection current|currents]] of [[Plasma (physics)|plasma]] in the Sun's [[convective zone]], directly below the photosphere. The grainy appearance of the photosphere is produced by the tops of these convective cells; this pattern is referred to as '''granulation'''.

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A typical granule has a diameter on the order of {{convert|1500|km}}<ref name="JBZ">{{cite book |title=Sunquakes: Probing the Interior of the Sun |publisher=Johns Hopkins University Press |first=Jack B. |last=Zirker |page=2 |date=2003 |isbn=0-8018-7419-X |oclc=919928822}}</ref> and lasts 8 to 20 minutes before dissipating.<ref>{{cite journal |title=Lifetime of Solar Granules |journal=[[The Astrophysical Journal]] |first1=J. |last1=Bahng |first2=M. |last2=Schwarzschild |name-list-style=amp |volume=134 |page=312 |date=September 1961 |doi=10.1086/147160 |bibcode=1961ApJ...134..312B|doi-access=free }}</ref> At any one time, the [[Sun]]'s surface is covered by about 4 million granules. Below the photosphere is a layer of "[[Supergranulation|supergranules]]" up to {{convert|30000|km}} in diameter with lifespans of up to 24 hours.

A typical granule has a diameter on the order of {{convert|1500|km}}<ref name="JBZ">{{cite book |title=Sunquakes: Probing the Interior of the Sun |publisher=Johns Hopkins University Press |first=Jack B. |last=Zirker |page=2 |date=2003 |isbn=0-8018-7419-X |oclc=919928822}}</ref> and lasts 8 to 20 minutes before dissipating.<ref>{{cite journal |title=Lifetime of Solar Granules |journal=[[The Astrophysical Journal]] |first1=J. |last1=Bahng |first2=M. |last2=Schwarzschild |name-list-style=amp |volume=134 |page=312 |date=September 1961 |doi=10.1086/147160 |bibcode=1961ApJ...134..312B|doi-access=free }}</ref> At any one time, the [[Sun]]'s surface is covered by about 4 million granules. Below the photosphere is a layer of "[[Supergranulation|supergranules]]" up to {{convert|30000|km}} in diameter with lifespans of up to 24 hours.


== Gallery ==

<gallery mode=packed heights=200px style="text-align:left">

Granulation_Quiet_Sun_SST_25May2017.webm|Granulation motions on the Sun's surface observed by the [[Swedish Solar Telescope]]

Sunspot_SST_05Sep2016.png|Detailed view of a [[sunspot]] and surrounding solar surface. The dense pattern of cells (unrelated to the sunspot) is ''granulation''; the individual cells are ''granules''.

</gallery>



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== References ==

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