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HZE ion

HZE ions are the high-energy nuclei component of galactic cosmic rays (GCRs) that have an electric charge of +3 e or greater – that is, they must be the nuclei of elements that have an atomic number that is greater than that of helium.

Composition and abundance
HZE ions are rare compared to protons, for example, composing only 1% of GCRs versus 85% for protons. HZE ions, like other GCRs, travel near the speed of light. In addition to the HZE ions from cosmic sources, HZE ions are produced by the Sun. During solar flares and other solar storms, HZE ions are sometimes produced in small amounts, along with the more typical protons, : GCRs typically originate from outside the Solar System and within the Milky Way galaxy, but those from outside of the Milky Way consist mostly of highly energetic protons with a small component of HZE ions. GCR energy spectra peaks, with median energy peaks up to , and nuclei (with energies up to ) are important contributors to the dose equivalent. == Health concerns of HZE ions ==
Health concerns of HZE ions
Although HZE ions make up a small proportion of cosmic rays, their high charge and high energies cause them to contribute significantly to the overall biological impact of cosmic rays, making them as significant as protons in regard to biological impact. == See also ==
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