Time Variation of Primary Heavy Nuclei in Cosmic Radiation
- 15 September 1956
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 103 (6) , 1820-1824
- https://doi.org/10.1103/physrev.103.1820
Abstract
The time variation of heavy nuclei in the primary cosmic radiation was investigated by using the method of a moving-plate mechanism which was flown to an altitude of 100 000 feet by a Skyhook balloon. The results obtained clearly indicate a time variation of primary heavy nuclei . The variation is characterized by its maximum at around 9:00 a.m., having an amplitude of 34±7% at the maximum. Comparisons are made with other experimental data on the same subject and also with the neutron intensity variation on the same day at Climax, Colorado. Possible consequences of this rather large fluctuation of the primary heavy nuclei are discussed.
Keywords
This publication has 18 references indexed in Scilit:
- Primary Heavy NucleiPhysical Review B, 1954
- The Time Variation of Cosmic-Ray Heavy NucleiPhysical Review B, 1953
- Angular Distribution of Pions Scattered by HydrogenPhysical Review B, 1953
- The Heavy Nuclei of the Primary Cosmic RadiationPhysical Review B, 1951
- A Scintillation Counter Measurement of Heavy NucleiPhysical Review B, 1951
- Evidence for the Multiple Production of Mesons in a Single Nucleon-Nucleon CollisionPhysical Review B, 1950
- The Excited Nuclear State ofBe7Physical Review B, 1950
- The Intensity of Primary Heavy Nuclei in the Stratosphere at NightPhysical Review B, 1950
- A Study of Time-Variations in Cosmic-Ray Intensity at High AltitudesPhysical Review B, 1940
- New Evidence for a Change with Time of the Total Energy Brought into the Earth by Cosmic RaysPhysical Review B, 1939