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Veröffentlicht in:Physical Review (U.S.) Superseded in part by Phys.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
Hauptverfasser: Biswas, S., Lavakare, P. J., Neelakantan, K. A., Shukla, P. G.
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container_title Physical Review (U.S.) Superseded in part by Phys.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
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creator Biswas, S.
Lavakare, P. J.
Neelakantan, K. A.
Shukla, P. G.
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doi_str_mv 10.1103/PhysRev.118.591
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ispartof Physical Review (U.S.) Superseded in part by Phys.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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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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