File:Tormenta solar.jpg
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DescriptionTormenta solar.jpg |
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 |
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Date | |||||||
Source | http://sdo.gsfc.nasa.gov/firstlight/ | ||||||
Author | NASA/SDO AIA Team | ||||||
Permission (Reusing this file) |
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current | 23:32, 22 April 2010 | 1,200 × 1,600 (2.75 MB) | Manuelt15 (talk | contribs) | {{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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- شراره خورشیدی
- ویکیپدیا:گزیدن نگاره برگزیده/دسامبر-۲۰۱۲
- ویکیپدیا:نگاره روز/آوریل ۲۰۱۳
- ویکیپدیا:گزیدن نگاره برگزیده/Tormenta solar.jpg
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- الگو:نر محافظت شده/2013-04-20
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Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |