File:Cosmic ray flux versus particle energy.svg

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Cosmic_ray_flux_versus_particle_energy.svg‎ (SVG file, nominally 400 × 480 pixels, file size: 94 KB)

[edit] Summary

Description
English: 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
Français : Le flux de particules du rayonnement cosmique (incident au sommet de l'atmosphère terrestre, par unité de surface, par unité de temps et par unité d'angle solide et par intervalle d'énergie des particules incidentes de 1 gigaélectron-volt (1 GeV)) représenté en fonction de leur énergie.
Le flux des énergies les plus basses (zone jaune) sont principalement imputables à l'énergie solaire des rayons cosmiques, les énergies intermédiaires (en bleu) pour les rayons cosmiques galactiques, et plus hautes énergies (violet) à extragalactique des rayons cosmiques)
Date 12 January 2007(2007-01-12)
Source own work, after Swordy.[1]
Author Sven Lafebre

[edit] References

  1. ↑ S. Swordy, The energy spectra and anisotropies of cosmic rays, 2001, Space Science Reviews 99, pp85–94.

[edit] Licensing

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Date/TimeThumbnailDimensionsUserComment
current14:12, 12 January 2007Thumbnail for version as of 14:12, 12 January 2007400 × 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 2007Thumbnail for version as of 14:05, 12 January 2007400 × 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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