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[{VerifyArticle user='eertl' template='Standard' date='23. November 2014' page-date='2014' comment='Überprüft, nach Jaros, A., Nussbaumer, A., Nussbaumer, P., Physik compact. Basiswissen 7RG; Ranzini, G., Atlas des Universums. Sonnensystem-Galaxien-Sternbilder' funder='65' }]
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!!!License Information of Images on page
||Image Description||Credit||Artist||License Name||File
| | | | [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:72408main ACD97-0036-1.jpg
| The Wikimedia Commons logo, SVG version.| Original created by Reidab ( PNG version ) SVG version was created by Grunt and cleaned up by 3247 . Re-creation with SVG geometry features by Pumbaa , using a proper partial circle and SVG geometry features. (Former versions used to be slightly warped.)| Reidab , Grunt , 3247 , Pumbaa| [{Image src='https://www.austria-forum.org/cc/images/slim/by-sa.png' alt='CC BY-SA 3.0' align='center' link='https://www.austria-forum.org/cc/by-sa-30.html' target='_blank'}]| Datei:Commons-logo.svg
| Crepuscular rays. View from Beaucatcher Ridge, Asheville, N.C. Image ID: wea00170, Historic NWS Collection.| photolib.noaa.gov at the Wayback Machine (archived 2001-01-30)| Grant W. Goodge| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Crepuscular rays8 - NOAA.jpg
| Begriffsklärungs-Icon (Autor: Stephan Baum)| Eigenes Werk ( Originaltext: Own drawing by Stephan Baum ) Original Commons upload as File:Logo Begriffsklärung.png by Baumst on 2005-02-15| Stephan Baum| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Disambig-dark.svg
| Fraunhofer lines| http://history.nasa.gov/SP-402/ch2.htm http://history.nasa.gov/SP-402/p16b.jpg| NASA| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:FraunhoferLinesDiagram.jpg
| The chromosphere of the sun in H-alpha light, observed by the .| NASA| CWitte| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:HI6563 fulldisk.jpg
| | | | [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Helioseismology GOLFpmode.png
| | | | [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Helioseismology pmode1.png
| This image at the time of publication is the highest resolution image of the sun's surface ever taken, at 789 nanometers (nm). Features as small as 30km (18 miles) in size are observable for the first time. The image shows a pattern of turbulence of solar plasma, a super-heated gas. The cell-like structures, each about the size of Texas (approximately 700'000km 2 ), are the signature of a dynamic activity of heat from the inside of the sun to its surface. The solar material rising in the bright centers of “cells" then sinks becoming a darker less-hot material by convection. The smaller brighter (intercell) areas with the darker areas are indications of magnetic fields, thought to channel energy that becomes the outer layers of the solar atmosphere which is the corona| Daniel K. Inouye Solar Telescope High res URL ( archived link ) License details ( Archived URL ) Image URL ( Archived link ) Description ( Archived link ) Date taken ( Archived link )| NSO / AURA / NSF| [{Image src='https://www.austria-forum.org/cc/images/slim/by.png' alt='CC BY 4.0' align='center' link='https://www.austria-forum.org/cc/by-40.html' target='_blank'}]| Datei:Highest resolution photo of Sun (NSF) as of January 20, 2020.jpg
| In der Sonne brennt ein ständiges Feuer, verursacht durch Kernfusion: Dabei verschmelzen leichte Atomkerne zu schwereren chemischen Elementen. Bei diesem Prozess wird sehr viel Energie freigesetzt.| https://www.zdf.de/dokumentation/terra-x/kernfusion-in-der-sonne-creative-commons-clip-100.html| ZDF/Terra X plus/Bilderfest/Nina Beier/Benjamin Herzberger/Fabian Brokmeier/ Phillip Becker/Maximilian Heß https://www.weltderphysik.de/gebiet/universum/sterne/sonne/energieproduktion-in-der-sonne/| [{Image src='https://www.austria-forum.org/cc/images/slim/by.png' alt='CC BY 4.0' align='center' link='https://www.austria-forum.org/cc/by-40.html' target='_blank'}]| Datei:Kernfusion in der Sonne.webm
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