Concept information
TERME PRÉFÉRENTIEL
COSMIC RAYS
DÉFINITION
- High energy particles and photons emitted by stellar processes. The highest energies have been observed at 10*8 Tev and are believed to come from shocks emanating from galaxies. Solar cosmic rays are protons observed at 1 Gev, having been accelerated by shocks associated with solar flares.
CONCEPT GÉNÉRIQUE
URI
https://gcmd.earthdata.nasa.gov/kms/concept/e06822d8-b640-4d75-ac37-33ab3cc5e765
{{toUpperCase label}}
{{#each values }} {{! loop through ConceptPropertyValue objects }}
{{#if prefLabel }}
{{/if}}
{{/each}}
{{#if notation }}{{ notation }} {{/if}}{{ prefLabel }}
{{#ifDifferentLabelLang lang }} ({{ lang }}){{/ifDifferentLabelLang}}
{{#if vocabName }}
{{ vocabName }}
{{/if}}