Abstract
Analytical calculations have been done to estimate the energy spectra of the secondary electrons originated from the decay of charged and neutral pions initiated on the upper atmosphere from the primary nucleon–air interactions in the energy range (4–100) GeV. The calculations are valid up to an atmospheric depth of about (3.8–7.4) g.cm−2. The derived results are compared with the observed electron fluxes available from the balloon flight experiments of MASS2, HEAT, magnetic spectrometer system of Golden et al., instrument using scintillating fibers of Nishimura et al., and BETS.
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References
D. Muller and J. Tang: in Proc. 18th Int. Cosmic Ray Conf., Bangalore 1983 (Eds. N. Durgaprasad, S. Ramadurai, P.V. Ramana Murthy, M.V.S. Rao, and K. Sivaprasad), Tata Institute of Fundamental Research, Bombay, 1983, Vol. 2, p. 60.
B.G. Mauger and J.F. Ormes: in Proc. 18th Int. Cosmic Ray Conf., Bangalore 1983 (Eds. N. Durgaprasad, S. Ramadurai, P.V. Ramana Murthy, M.V.S. Rao, and K. Sivaprasad), Tata Institute of Fundamental Research, Bombay, 1983, Vol. 2, p. 65.
D.J. Van der Walt: in Proc. 22nd Int. Cosmic Ray Conf., Dublin 1991 (Eds. M. Cawley, L.O'C. Drury, D.J. Feagan, D. O'Sullivan, N.A. Porter, J.J. Quenby, A.A. Watson), Reprint Ltd., Ireland, 1991, Vol. 2, p. 141.
K.K. Tang: Astrophys. J. 278 (1984) 881.
R.L. Golden, B.J. Mauger, G.D. Badhwar et al.: Astrophys. J. 287 (1984) 622.
J. Nishimura, T. Kobayashi et al.: in Proc. 25th Int. Cosmic Ray Conf., Durban 1997 (Eds. M.S. Potgieter, B.C. Raubenheiner, and D.J. Van der Walt), Wesprint, Potchefstrom, 1997, Vol. 4, p. 233.
V.S. Ptuskin and J.F. Ormes: in Proc. 24th Int. Cosmic Ray Conf., Rome 1995 (Ed. Nunzio Iucci), University of Roma "La Sapienza", Rome, 1995, Vol. 3, p. 56.
G. Basini, R. Bellotti, F. Bongiorno et al.: in Proc. 24th Int. Cosmic Ray Conf., Rome 1995 (Ed. Nunzio Iucci), University of Roma "La Sapienza", Rome, 1995, Vol. 3, p. 1.
S. Torri, J. Nishimura, K. Kasahara et al.: Proc. SPIE 2806 (1996) 145.
R.L. Golden et al.: Astrophys. J. 436 (1994) 769.
G.D. Badhwar, R.L. Golden, M.L. Brown, J.L. Lacy: Astrophys. Space Sci. 37 (1975) 283.
S.D. Verma: Proc. Ind. Acad. Sci. 66 (1967) 125.
R.K. Saha, R. Majumdar, P. 6Pal, and D.P. Bhattacharyya: Mod. Phys. Lett. 13 (1998) 1997.
A. Dar: Cosmic ray muons at ground level and deep underground, Technion Physics Report No. 84-41, 1984.
R.P. Feynman: Phys. Rev. Lett. 23 (1969) 1415.
G.A. de Nolfo et al.: in Proc. 25th Int. Cosmic Ray Conf., Durban 1997 (Eds. M.S. Potgieter, B.C. Raubenheiner, and D.J. Van der Walt), Wesprint, Potchefstrom, 1997, Vol. 2, p. 373.
S.W. Barwick et al.: J. Geophys. Res. 103 (1998), No. A3, 4817.
D. Muller, S.W. Barwick, and J.J. Beatty: in Proc. 24th Int. Cosmic Ray Conf., Rome 1995 (Ed. Nunzio Iucci), University of Roma "La Sapienza", Rome, 1995, Vol. 3, p. 13
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Saha, R., Majumdar, R., Pal, P. et al. Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8–7.4)g.cm−2 . Czechoslovak Journal of Physics 49, 1503–1507 (1999). https://doi.org/10.1023/A:1021118314302
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DOI: https://doi.org/10.1023/A:1021118314302