Charge composition of primary cosmic ray nuclei with Z greater than or equal to 2 in energy region greater than or equal to 2 TeV

Details Charge composition of primary cosmic ray nuclei with Z greater than or equal to 2 in energy region greater than or equal to 2 TeV Charge composition of primary cosmic ray nuclei with Z greater than or equal to 2 in energy region greater than or equal to 2 TeV

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rpsct...3...19i&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 19 (SEE N88-30498 24-88) Transl. into ENGLISH from Kosmicheskiye Issle

Computer Science

Charge Distribution, Heavy Nuclei, Primary Cosmic Rays, Spaceborne Experiments, Data Processing, Energy Distribution, Satellite-Borne Instruments

Scientific paper

An experiment to study cosmic ray particles with energies approximately 1 TeV or greater was carried out in 1984 using the Sokol instrument carried aboard the Cosmos-1543. Particle energy was measured using an ionization calorimeter and particle charge was measured using Cerenkov detectors situated above it. Protons and alpha particles are reliably separated by DZ-1 detectors. The fraction of alpha particles among the registered protons and the fraction of protons among the alpha particles does not exceed a few percent. The charge distribution of nuclei with z greater than 5 for the energy interval 1 to 10 TeV and the charge distribution of nuclei with z greater than or equal to 2 for an energy greater than or equal to 2 TeV are shown graphically. With transition to energies greater than or equal to 2 TeV the charge composition of primary cosmic ray nuclei with z greater than or equal to 2 does not experience significant changes.

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