File:Images of Type III Solar Radio Bursts.png
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Summary
| Description |
English: Murchison Widefield Array images of the background solar emission at 240 MHz (grayscale) with color contours showing the locations of Type III solar radio bursts at a range of frequencies. The peak burst intensities are hundreds of times greater than the background, and the lower-frequency contours appear at larger distances from the surface (indicated by the solid circle) because the bursts are produced by a beam of electrons that travels away from the Sun, exciting radio emission of lower and lower frequencies as it gets farther away. |
| Date | |
| Source | Own work |
| Author | Patrick McCauley Mccauley.pi |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 20:46, 24 January 2021 |  | 1,054 × 507 (203 KB) | Mccauley.pi | Cross-wiki upload from en.wikipedia.org |
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