File:SDO 20101129 005133 4096 0304 (AIA).jpg

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DescriptionSDO 20101129 005133 4096 0304 (AIA).jpg	English: AIA 0304 channel is especially good at showing areas where cooler dense plumes of plasma (filaments and prominences) are located above the visible surface of the Sun. Many of these features either can't be seen or appear as dark lines in the other channels. The bright areas show places where the plasma has a high density. Where: Upper chromosphere and lower transition region Wavelength: 304 angstroms (0.0000000304 m) = Extreme Ultraviolet Primary ions seen: singly ionized helium (He II) Characteristic temperature: 50,000 K (90,000 F)
Date	Taken on 29 November 2010, 00:51:33
Source	20101129_005133_4096_0304
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

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Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory

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