File:Cosmic_ray_flux_versus_particle_energy.svg
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Summary
DescriptionCosmic ray flux versus particle energy.svg |
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 aux rayons cosmiques solaires, les énergies intermédiaires (en bleu) aux rayons cosmiques galactiques, et les plus hautes énergies (violet) aux rayons cosmiques extragalactiques |
Date | |
Source | own work, after Swordy[1] and De Angelis[2] |
Author | Sven Lafebre |
References
- ↑ S. Swordy, The energy spectra and anisotropies of cosmic rays, 2001, Space Science Reviews 99, pp85–94.
- ↑ A. de Angelis and M. Pimenta, Introduction to particle and astroparticle physics (Multimessenger astronomy and its particle physics foundations), Springer 2018, p577.
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8 January 2019
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78a66147ff4610e2ab092f4e7059c9b4329028b2
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 10:31, 15 February 2019 | 512 × 614 (113 KB) | Cherkash | an updated 2018 version uploaded based on the original author's request (see [https://commons.wikimedia.org/wiki/Commons:Help_desk/Archive/2019/01#New_version_of_%22Cosmic_ray_flux_versus_particle_energy%22_image here]) | |
14:12, 12 January 2007 | 400 × 480 (94 KB) | Svenlafe~commonswiki | == 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~commonswiki | {{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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