Difference between revisions of "File:Proton Energy Spectra Space Radiation.png"

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Data from D.J. McComas et al., "Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation", (2014) Space Science Reviews 204. DOI 10.1007/s11214-014-0059-1
Data from D.J. McComas et al., "Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation", (2014) Space Science Reviews 204. DOI 10.1007/s11214-014-0059-1
Figure drawn by Luke Campbell, used with permission.

Latest revision as of 11:10, 28 April 2024

Summary

Proton energy spectra at 1 AU, showing the increase in solar energetic particles during solar particle events. SEP = solar energetic particle, GCR = galactic cosmic ray.

Data from D.J. McComas et al., "Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation", (2014) Space Science Reviews 204. DOI 10.1007/s11214-014-0059-1

Figure drawn by Luke Campbell, used with permission.

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current22:47, 19 February 2024Thumbnail for version as of 22:47, 19 February 2024850 × 814 (161 KB)Lwcamp (talk | contribs)Proton energy spectra at 1 AU, showing the increase in solar energetic particles during solar particle events. SEP = solar energetic particle, GCR = galactic cosmic ray.

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