Isotopic Composition of the Primary Cosmic Radiation
| Author | : Philip M. Dauber |
| Publisher | : |
| Total Pages | : 302 |
| Release | : 1971 |
| Genre | : Cosmic rays |
| ISBN | : |
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Measurement of the Isotopic Composition of the Primary Cosmic Radiation for the Elements B-Ne
| Author | : Christer Bjarle |
| Publisher | : |
| Total Pages | : 12 |
| Release | : 1977 |
| Genre | : |
| ISBN | : |
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A Measurement of the Carbon Isotopic Composition in Primary Cosmic Radiation
| Author | : Christer Bjarle |
| Publisher | : |
| Total Pages | : 14 |
| Release | : 1975 |
| Genre | : |
| ISBN | : |
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Isotopic Composition of the Primary Cosmic Radiation
| Author | : Danish Space Research Institute |
| Publisher | : |
| Total Pages | : 294 |
| Release | : 1971 |
| Genre | : |
| ISBN | : |
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The Isotopic Composition of Low Energy Helium Nuclei in Primary Cosmic Radiation
| Author | : M. V. K. Appa Rao |
| Publisher | : |
| Total Pages | : 124 |
| Release | : 1962 |
| Genre | : |
| ISBN | : |
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Isotopic Composition of the Primary Cosmic Radiation
| Author | : Philip M. Dauber |
| Publisher | : |
| Total Pages | : |
| Release | : 1971 |
| Genre | : |
| ISBN | : |
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Proceedings of a Symposium on Isotopic Composition of the Primary Cosmic Radiation. Lyngby. March, 1971
| Author | : Philip M. Dauber |
| Publisher | : |
| Total Pages | : 294 |
| Release | : 1971 |
| Genre | : |
| ISBN | : |
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A Study of the Isotopic Composition of Low-energy Hydrogen and Helium Nuclei in the Primary Cosmic Radiation
| Author | : Gautam Dev Badhwar |
| Publisher | : |
| Total Pages | : 250 |
| Release | : 1967 |
| Genre | : |
| ISBN | : |
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The Isotopic Composition and the Energy Spectrum of Low Energy Helium Nuclei in Primary Cosmic Radiation
| Author | : Prabhakar J. Lavakare |
| Publisher | : |
| Total Pages | : 198 |
| Release | : 1964 |
| Genre | : |
| ISBN | : |
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Isotopic Composition of Low Energy Hydrogen Nuclei in the Primary Cosmic Radiation
| Author | : G. D. Badhwar |
| Publisher | : |
| Total Pages | : 18 |
| Release | : 1964 |
| Genre | : Cosmic rays |
| ISBN | : |
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The abundance of low energy deuterons and tritons was determined in a nuclear emulsion stack exposed at Fort Churchill, Manitoba, Canada on August 4, 1962 under 4.2 g/sq cm of residual atmosphere. Using the grain density vs. residual range method for the identification of tracks produced by particles, the differential flux of deuterons and tritons was determined. The results appear to be consistent with the absence of deuterons and tritons in the primary cosmic radiation. An upper limit on the amount of hydrogen traversed by low energy cosmic ray particles has been placed. (Author).
