Skip to main content
Log in

Cosmic-ray intensity measurements deep undergound at depths of (800÷8400) m w.e.

  • Published:
Il Nuovo Cimento (1955-1965)

Summary

An experiment has been carried out to investigate the variation of vertical cosmic-ray intensity with depth in the range (800÷8400) m w.e. Counter telescopes with plastic scintillator layers and Geiger counter trays, kept in the horizontal plane and in coincidence, were employed. The experiment was carried out in the Kolar Gold Fields (Mysore State, India). The results obtained at depths of 816, 1812, 3410, 4280, 6380 and 8400 m w.e. are given.

Riassunto

Si è effettuato un esperimento per studiare la variazione dell’intensità verticale dei raggi cosmici nell’intervallo (800÷8400) m a.e. Si sono adoperati telescopi di contatori con strati di scintillatori plastici e vassoi di contatori di Geiger posti orizzontalmente e in coincidenza. L’esperimento fu eseguito nei Kolar Gold Fields (Stato di Mysore). Si riportano i risultati ottenuti alle profondità di 816, 1812, 3410, 4280, 6380 e 8400 m a.e.

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.

Similar content being viewed by others

References

  1. P. H. Barrett, L. M. Bollinger, G. Cocconi, Y. Eisenberg andK. Greisen:Rev. Mod. Phys.,24, 133 (1952).

    Article  ADS  Google Scholar 

  2. E. P. George:Prog. in Cosmic Ray Physics, Vol.1 (1952).

  3. B. V. Sreekantan andS. Naranan:Proc. Ind. Acad. Sci.,36, 97 (1952);B. V. Sreekantan, S. Naranan andP. V. Ramana Murthy:Proc. Ind. Acad. Sci.,43, 113 (1956).

    Google Scholar 

  4. J. C. Barton:Phil. Mag.,6, 1271 (1961).

    Article  ADS  Google Scholar 

  5. Y. Miyazaki:Phys. Rev.,76, 1733 (1949).

    Article  MathSciNet  ADS  Google Scholar 

  6. L. M. Bollinger:Ph. D. Thesis, Cornell University (1951). Relevant results from this thesis are easily accessible in the references (1,15).

  7. S. Miyake, V. S. Narasimham andP. V. Ramana Murthy:Proc. Int. Conj. on Cosmic Rays and the Earth Storms, inJourn. Phys. Soc. Japan, Supplement A III,17, 318 (1962).

    Google Scholar 

  8. N. R. Parsons:Rev. Sci. Instr.,28, 265 (1957);D. A. Tidman andK. W. Ogilvie:Nuovo Cimento,6, 735 (1957);R. P. Kane andU. R. Rao:Proc. Ind. Acad. Sci., A47, 30 (1958);D. Stern:Nuovo Cimento,16, 153 (1960).

    Article  ADS  Google Scholar 

  9. C. A. Randall andW. E. Hazen:Nuovo Cimento,8, 878 (1958).

    Article  MATH  Google Scholar 

  10. J. C. Barton andE. G. Michaelis:Proc. Phys. Soc.,77, 377 (1961).

    Article  ADS  Google Scholar 

  11. M. G. K. Menon, P. V. Ramana Murthy, B. V. Sreekantan andS. Miyake:Nuovo Cimento,30, 1208 (1963).

    Article  MATH  Google Scholar 

  12. V. C. Wilson:Phys. Rev.,53, 337 (1938).

    Article  ADS  Google Scholar 

  13. J. Clay andA. von Gemert:Physica,6, 497 (1939).

    Article  ADS  Google Scholar 

  14. C. A. Randall andW. E. Hazen:Phys. Rev.,81, 144 (1951).

    Article  ADS  Google Scholar 

  15. J. Pine, R. J. Davisson andK. Greisen:Proc. Moscow Conf., Vol.1, 295 (1960).

    Google Scholar 

  16. T. Pryor:Notes on the Geology of K.G.F. (unpublished) (1950).

Download references

Author information

Authors and Affiliations

Authors

Additional information

1 m w.e. is used to denote 100 g cm−2 of matter (rock).

Rights and permissions

Reprints and permissions

About this article

Cite this article

Miyake, S., Narasimham, V.S. & Ramana Murthy, P.V. Cosmic-ray intensity measurements deep undergound at depths of (800÷8400) m w.e.. Nuovo Cim 32, 1505–1523 (1964). https://doi.org/10.1007/BF02732788

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02732788

Navigation