Gradients of galactic cosmic rays in the ecliptic plane at the maximum of the 19th solar cycle studied on the basis of data on the radioactivity of the Bruderheim chondrite

Details Gradients of galactic cosmic rays in the ecliptic plane at the maximum of the 19th solar cycle studied on the basis of data on the radioactivity of the Bruderheim chondrite Gradients of galactic cosmic rays in the ecliptic plane at the maximum of the 19th solar cycle studied on the basis of data on the radioactivity of the Bruderheim chondrite

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980izssr..44.2552l&link_type=abstract

(Seminar po Vzaimodeistviiu Kosmicheskikh Luchei so Sredoi, Leningrad, USSR, Nov. 30-Dec. 2, 1979.) Akademiia Nauk SSSR, Izvesti

Physics

Chondrites, Cosmic Rays, Galactic Radiation, Radioactivity, Solar Activity Effects, Radiation Measurement, Radioactive Isotopes, Solar Cycles

Scientific paper

An analysis is presented of the radioactivity of the cosmogenic isotopes of the Bruderheim chondrite which fell on March 4, 1960 and the orbit of which lay in the ecliptic plane. It is found that gradients of galactic cosmic rays (R greater than 0.5 GV) in the ecliptic plane amounted to 50-70% for 1 AU at the maximum (1956-1959) of the 19th solar cycle. The magnitude of the gradients is determined by the level of solar modulation and by their heliocentric distance and solar latitude.

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