A study of solar modulation of medium energy primary cosmic ray nuclei

Details A study of solar modulation of medium energy primary cosmic ray nuclei A study of solar modulation of medium energy primary cosmic ray nuclei

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985japa....6...57d&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 6, March 1985, p. 57-60. Research supported by the University Grant

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Energy Spectra, Heavy Nuclei, Primary Cosmic Rays, Solar Activity Effects, Balloon Sounding, Solar Cycles

Scientific paper

The energy spectra of primary cosmic rays were studied in the energy interval 150 to 450 MeV/nucl by using a balloon-borne cellulose-nitrate solid-state plastic detector. Effects of solar modulation were studied using the theoretical spectrum of H1 nuclei near the solar minimum in 1964 as the demodulated spectrum. The "force-field" potential which fit the experimental results was estimated to be 270 MeV/nucl.

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