Cosmic-Ray Increase at High Altitude on February 23, 1956

Details Cosmic-Ray Increase at High Altitude on February 23, 1956 Cosmic-Ray Increase at High Altitude on February 23, 1956

Oct 1956

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1956phrv..104..220w&link_type=abstract

Physical Review, vol. 104, Issue 1, pp. 220-220

Physics

2

Scientific paper

A vertical telescope with a stopping power of 22 g/cm2 was flown to an atmospheric depth of 10 g/cm2 at Minneapolis seventeen hours after the beginning of the giant solar flare and cosmic ray increase of February 23, 1956. The cosmic-ray intensity was normal below 300 g/cm2, but at 10 g/cm2 was five times the normal intensity at Minneapolis. The particles apparently have energies less than one Bev, presumably originated near the sun and reached the earth by scattering from magnetic fields near the solar system.

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