Evidence for a Forbush Type of Decrease in the Intensity of Heavy Nuclei of the Primary Cosmic Radiation
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Veröffentlicht in: | Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D, 1960-04, Vol.118 (2), p.591-593 |
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container_title | Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D |
container_volume | 118 |
creator | Biswas, S. Lavakare, P. J. Neelakantan, K. A. Shukla, P. G. |
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doi_str_mv | 10.1103/PhysRev.118.591 |
format | Article |
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ispartof | Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D, 1960-04, Vol.118 (2), p.591-593 |
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language | eng |
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source | American Physical Society Journals |
subjects | BALLOONS COSMIC RADIATION DISTRIBUTION ELECTRIC CHARGES ENERGY ENERGY RANGE FORBUSH DEPRESSION LEVELS MAGNETIC FIELDS MEASURED VALUES NUCLEAR EMULSIONS NUCLEI PARTICLE TRACKS PHYSICS SPECTRA STRATOSPHERE VARIATIONS C |
title | Evidence for a Forbush Type of Decrease in the Intensity of Heavy Nuclei of the Primary Cosmic Radiation |
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