Il Nuovo Cimento (1955-1965)

, Volume 16, Issue 4, pp 762–764 | Cite as

Mean free path of primary cosmic rays in the atmosphere

  • R. W. Williams
Lettere Alla Redazione


Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.


  1. (1).
    A. Subramanian andS. D. Verma Nuovo Cimento,13, 572 (1959).CrossRefGoogle Scholar
  2. (2).
    R. W. Williams:Phys. Rev.,98, 1387 (1955).ADSCrossRefGoogle Scholar
  3. (3).
    R. M. Kalbach, J. J. Lord andC. H. Tsao:Phys. Rev.,113, 325 (1959);M. Blue andJ. J. Lord: to be published.ADSCrossRefGoogle Scholar
  4. (4).
    N. P. Bogachev, S. A. Bonjatov, Ju. P. Merekov andV. M. Siderov:Dokl. Akad. Nauk. SSSR,121, 617 (1958). A slightly higher value (25 mb) is quoted in the proceedings of the 1958 Geneva Conference.Google Scholar
  5. (5).
    A. E. Brenner andR. W. Williams:Phys. Rev.,106, 1020 (1957).ADSCrossRefGoogle Scholar
  6. (6).
    U. Meyer-Berkhout, K. W. Ford andA. E. S. Green:Ann. of Phys.,8, 119 (1959).ADSCrossRefGoogle Scholar
  7. (7).
    J. Cronin, R. Cool andA. Abachian:Phys. Rev.,107, 1121 (1957).ADSCrossRefGoogle Scholar
  8. (8).
    J. Atkinson, W. Hess, V. Perez-Mendez andR. Wallace:Phys. Rev. Lett.,2, 168 (1959).ADSCrossRefGoogle Scholar

Copyright information

© Società Italiana di Fisica 1960

Authors and Affiliations

  • R. W. Williams
    • 1
  1. 1.Physics DepartmentUniversity of WashingtonSeattle

Personalised recommendations