Ultra-heavy cosmic ray studies with Ariel VI

Details Ultra-heavy cosmic ray studies with Ariel VI Ultra-heavy cosmic ray studies with Ariel VI

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.291...45f&link_type=abstract

Nature, vol. 291, May 7, 1981, p. 45-47.

Physics

13

Abundance, Ariel Satellites, Cosmic Rays, Heavy Nuclei, Radiation Spectra, Scintillation Counters, Geomagnetism, Iron, Nickel, Skylab Program, Solar System, Zinc

Scientific paper

The satellite Ariel VI was launched on June 3, 1979 into a near-circular 625 km, 55 deg inclination orbit. The Bristol experiment on board is of a novel design using a spherical gas scintillation chamber with an integral plastic Cerenkov element. The data presented here were collected during an exposure of approximately 360 sq m sr days with essentially 100% recording efficiency for events with Z greater than or equal to

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