File:SDO 20190209 000239 4096 1600 (AIA).jpg

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DescriptionSDO 20190209 000239 4096 1600 (AIA).jpg	English: AIA 1600 channel (as well as AIA 1700) often shows a web-like pattern of bright areas that highlight places where bundles of magnetic fields lines are concentrated. However, small areas with a lot of field lines will appear black, usually near sunspots and active regions. Where: Transition region and upper photosphere Wavelength: 1600 angstroms (0.00000016 m) = Far Ultraviolet Primary ions seen: thrice ionized carbon (C IV) and Continuum Characteristic temperatures: 6,000 K (11,000 F), and 100,000 K (180,000 F)
Date	Taken on 9 February 2019, 00:02:39
Source	20190209_000239_4096_1600
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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