Primary Heavy Nuclei
- 1 August 1954
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 95 (3) , 782-792
- https://doi.org/10.1103/PhysRev.95.782
Abstract
Primary cosmic-ray nuclei of were observed in a balloon-borne cloud chamber. The chamber was triggered by events with ionization loss ≥6 minimum in each of three proportional counters, arranged in a telescope. Proportional counter pulse amplitudes were recorded by a neon bulb system.
Keywords
This publication has 29 references indexed in Scilit:
- Neutral-to-Charge Ratio in High-Energy InteractionsPhysical Review B, 1954
- The Abundance of Beryllium in the Sun.The Astrophysical Journal, 1954
- Production of Fast Lithium, Beryllium, Boron Fragments from Interactions of Primary Cosmic-Ray NucleiPhysical Review B, 1953
- The Energy Spectrum of Primary Cosmic RadiationPhysical Review B, 1952
- Abundance of Lithium, Beryllium, Boron, and Other Light Nuclei in the Primary Cosmic Radiation and the Problem of Cosmic-Ray OriginPhysical Review B, 1950
- A Directional and Latitude Survey of Cosmic Rays at High AltitudesPhysical Review B, 1950
- Solar Magnetic Moment and Diurnal Variation in Intensity of Cosmic RadiationPhysical Review B, 1950
- Upper Limits on the Abundances of Interstellar li and Be.The Astrophysical Journal, 1949
- On the Density Distribution and Chemical Composition of the Interstellar Gas.The Astrophysical Journal, 1948
- Evidence for Heavy Nuclei in the Primary Cosmic RadiationPhysical Review B, 1948