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Original file (4,500 × 4,500 pixels, file size: 7.05 MB, MIME type: image/jpeg)
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Summary
| Description |
This is a false-color, 3-layer composite from the TRACE observatory showing the solar corona: the blue, green, and red channels show the 171Å, 195Å, and 284Å, respectively. These TRACE filters are most sensitive to emission from 1, 1.5, and 2 million degree plasma, thus showing the entire corona and detail of coronal loops in the lower solar atmosphere). The image shows the corona for a moderately active Sun, with some (red) hot active regions in both hemispheres, surrounded by the (blue/green) cooler plasma of the quiet-Sun corona. Notice the multitude of relatively cool loops connecting the active regions on both hemispheres. |
| Date | |
| Source | [1] → [2] |
| Author | Unknown author |
| Other versions |
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![[2]](https://trace.lmsal.com/POD/images/FDM_4500_3EUV_19990802.jpg){kind=link}
Licensing
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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 | 14:47, 30 December 2010 | | 4,500 × 4,500 (7.05 MB) | Saibo | full res from src |
| 16:43, 29 April 2008 |  | 1,500 × 1,500 (669 KB) | Henrykus | {{Information |Description= This is a false-color, 3-layer composite from the TRACE observatory: the blue, green, and red channels show the 171Å, 195Å, and 284Å, respectively. These TRACE filters are most sensitive to emission from 1, 1.5, and |
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