Long-term variations of cosmic rays

Details Long-term variations of cosmic rays Long-term variations of cosmic rays

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..514b&link_type=abstract

(Mezhdunarodnyi Seminar po Korpuskuliarnye Potoki Solntsa i Radiatsionnye Poiasa Zemli i Iupitera, 7th, Leningrad, USSR, May 25-

Computer Science

Galactic Radiation, Secular Variations, Solar Cosmic Rays, Solar Wind, Aluminum 26, Lunar Rocks, Manganese Isotopes, Meteoritic Composition, Rare Gases

Scientific paper

The long term variations of the intensity of solar cosmic rays, galactic cosmic rays, and the solar wind were studied on the basis of radioisotope data. Data concerning Al-26/Mn-53 formed in lunar rocks by solar protons show a slight increase in the intensity of flare protons over the past million years. Meteoritic radioisotope data show that the mean intensity of galactic cosmic rays has remained virtually unchanged over the past million years. Long-term variations of the solar wind were studied on the basis of data on rare gas isotopes in lunar rocks.

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