Enhanced Emission of Iron Nuclei in Solar Flares

Details Enhanced Emission of Iron Nuclei in Solar Flares Enhanced Emission of Iron Nuclei in Solar Flares

Apr 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971phrvl..26..916p&link_type=abstract

Physical Review Letters, vol. 26, Issue 15, pp. 916-919

Physics

43

Scientific paper

Etched tracks in an Apollo-12 spacecraft window and a Surveyor-3 camera-lens filter give the interplanetary Fe energy spectra from ~1 to ~30 MeV/nucleon during 1967-1969. The strongly energy-dependent Fe/He ratio suggests that heavy nuclei are preferentially emitted from accelerating regions because of their low ionization state and high magnetic rigidity. The Fe fluxes give rise to extremely high track densities that we have observed in lunar soil.

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