Skip to main content
Log in

The influence of isotopic composition on the maximum in the cosmic ray energy spectra

  • Lettere Alla Redazione
  • Published:
Il Nuovo Cimento (1955-1965)

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

References

  1. F. B. Macdonald andW. R. Webber:Phys. Rev.,115, 194 (1959).

    Article  ADS  Google Scholar 

  2. F. B. Macdonald:Phys. Rev.,116, 462 (1959).

    Article  ADS  Google Scholar 

  3. P. H. Fowler andC. J. Waddington:Phil. May.,1, 637 (1956).

    Article  ADS  Google Scholar 

  4. P. H. Fowler, P. S. Freirr andE. P. Ney:Suppl. Nvovo Cimento,8, 492 (1958).

    Article  Google Scholar 

  5. P. S. Freier, E. P. Ney, J. E. Naugle andG. W. Anderson:Phys. Rev.,79, 206 (1950).

    Article  Google Scholar 

  6. H. Aizu, Y. Fujimoto, S. Hasegawa, M. Koshiba, I. Mito, J. Nishimura, K. Yokoi andM. Schein:Phys. Rev.,116, 436 (1959) andProc. Moscow Cosmic Ray Conf., vol.3 (1959)

    Article  ADS  Google Scholar 

  7. K. Yokoi: private Communication.

  8. A. Engler, M. F. Kaplon, A. Kernan, J. Klarmann, C. E. Fichtel. andM. W. Friedlander: submitted toNuovo Cimento.

  9. A. Engler, F. Foster, T. L. Green andJ. Mulvey: private Communication.

  10. S. F. Singer:Suppl. Nuovo Cimento,8, 342 (1958).

    Article  Google Scholar 

  11. M. V. K. Appa Rao andM. F. Kaplon: to be published.

  12. M. V. K. Appa Rao: to appear inphys. Rev.

  13. M. V. K. Appa Rao: private communication.

Download references

Author information

Authors and Affiliations

Authors

Additional information

This research is supported in part by theOffice of Scientific Research. USAF.

On leave of absence from Tata Institute of Fundamental Research, Bombay, India.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Rao, M.V.K.A., Kaplon, M.F. The influence of isotopic composition on the maximum in the cosmic ray energy spectra. Nuovo Cim 21, 369–372 (1961). https://doi.org/10.1007/BF02832562

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02832562

Navigation