File:Tormenta solar.jpg

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Description

English: Solar eruption, extreme ultraviolet emission line is from singly ionized Helium, or He II, and corresponds to a temperature of approx. 50,000 degrees Celsius

Date

30 March 2010

Source

http://sdo.gsfc.nasa.gov/firstlight/

Author

NASA/SDO AIA Team

Permission
(Reusing this file)

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	00:32, 23 April 2010		1,200 × 1,600 (2.75 MB)	wikimediacommons>Manuelt15	{{Information \|Description={{en\|1=Solar eruption, extreme ultraviolet emission line is from singly ionized Helium, or He II, and corresponds to a temperature of approx. 50,000 degrees Celsius}} \|Source=http://sdo.gsfc.nasa.gov/firstlight/ \|Author=NASA/SDO

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Chemicals/Heliums

File:Tormenta solar.jpg

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30 March 2010

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File:Tormenta solar.jpg

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inception

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media type

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File history

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