Fasciculus:Cosmic ray flux versus particle energy.svg

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Summarium

Descriptio
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
Datum
Fons own work, after Swordy[1] and De Angelis[2]
Auctor Sven Lafebre

References

  1. ↑ S. Swordy, The energy spectra and anisotropies of cosmic rays, 2001, Space Science Reviews 99, pp85–94.
  2. ↑ 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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This file is licensed under the Creative Commons Attribution-Share Alike 2.5 Generic, 2.0 Generic and 1.0 Generic license.
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  • to remix – to adapt the work
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Graph of cosmic flux versus particle energy

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recentissima10:31, 15 Februarii 2019Minutum speculum redactionis 10:31, 15 Februarii 2019 factae512 × 614 (113 chiliocteti)Cherkashan 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 Ianuarii 2007Minutum speculum redactionis 14:12, 12 Ianuarii 2007 factae400 × 480 (94 chiliocteti)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 Ianuarii 2007Minutum speculum redactionis 14:05, 12 Ianuarii 2007 factae400 × 480 (26 chiliocteti)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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