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Summary
| Description |
The flux of cosmic ray particles as a function of their energy. The flux for the lowest energies (yellow zone) are mainly attributed to solar cosmic rays, intermediate energies (blue) to galactic cosmic rays, and highest energies (purple) to extragalactic cosmic rays. |
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| Source |
own work, after Swordy.[1] |
| Date |
2007-01-12 |
| Author |
Sven Lafebre |
| Permission (Reusing this image) |
see below |
References
- ↑ S. Swordy, The energy spectra and anisotropies of cosmic rays, 2001, Space Science Reviews 99, pp85–94.
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File history
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| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 14:12, 12 January 2007 | 400×480 (94 KB) | Svenlafe | (== Summary == {{Information |Description=The flux of cosmic ray particles as a function of their energy. The flux for the lowest energies (yellow zone) are mainly attributed to solar cosmic rays, intermediate energies (blue) to galactic cosmic rays, and h) |
| 14:05, 12 January 2007 | 400×480 (26 KB) | Svenlafe | ({{Information |Description=The flux of cosmic ray particles as a function of their energy. The flux for the lowest energies (yellow zone) are mainly attributed to solar cosmic rays, intermediate energies (blue) to galactic cosmic rays, and highest energie) |
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