Energy Spectrum of Primary Cosmic Rays Between 10**14.5-ev and 10**18-ev
Jun, 1984
30 pages
Published in:
- J.Phys.G 10 (1984) 1295
Report number:
- ICR-116-84-5
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Abstract: (IOP)
Size spectra of electrons (Ne) and muons (Nmu ) are obtained from the Akeno extensive air-shower experiment. The primary spectrum estimated from each spectrum is the same and is expressed by J(E0)dE0(4.0-5.0)*10-23(E0/1015.67)- gamma dE0 m-2 s-1 sr-1 where gamma =2.62+or-0.12 below and gamma =3.02+or-0.05 above 1015.67 eV. There is no other significant change of slope in either the electron or the muon size spectrum beyond the corresponding energy 1015.67 eV.- COSMIC RADIATION: PRIMARY
- SHOWERS: AIR
- ELECTRON: COSMIC RADIATION
- MUON: COSMIC RADIATION
- DENSITY
- ENERGY SPECTRUM
- EXPERIMENTAL RESULTS
- ELECTRON: SPATIAL DISTRIBUTION
- MUON: SPATIAL DISTRIBUTION
- SCINTILLATION COUNTER: EXPERIMENTAL RESULTS
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