File:SDO 20121129 1024 0304 (AIA).ogv
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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 2012 |
| Source | 20121129_1024_0304 |
| Author | Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams. |
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This media is a product of the Solar Dynamics Observatory Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory |
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This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: 20121129_1024_0304. This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing. Other languages:
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:59, 21 April 2024 | 5.7 s, 1,024 × 1,024 (13.59 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2012/11/29/20121129_1024_0304.ogv via Commons:Spacemedia |
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